The galaxy presents as a largely featureless elliptical-type system. It exhibits a generally smooth and rounded morphology, with no discernible spiral arms or a distinct disk structure visible in the image. The color profile suggests a mature stellar population. The central region displays a concentrated, bright core, indicative of a significant bulge component and possibly a supermassive black hole. The outer regions gradually fade in intensity, suggesting a decreasing stellar density with radial distance. There is a hint of minor asymmetry that could be related to recent interactions with another galaxy, but no major disturbances are readily apparent. Overall, the galaxy appears to be a relatively evolved and quiescent system, likely exhibiting low rates of star formation. The galaxy's color suggests that it is more abundant with older stars in the redder region of the spectrum, indicating that it may be nearing the end of its life cycle and/or the presence of dust. The color gradient suggests a higher density of older stars in the galactic bulge. The lack of visible dust lanes, HII regions, or blue stars further supports this hypothesis.
