The galaxy presents as an elliptical morphology, appearing largely smooth and relatively featureless in this image. It exhibits a concentrated central bulge, with the light intensity decreasing gradually towards the outer edges. The galaxy's color profile suggests an older stellar population, with a distinct yellow-orange hue. There is no apparent spiral arm structure or significant dust lane obscuration visible. The overall shape is slightly elongated, deviating somewhat from a perfect circular form. There is no obvious evidence of active galactic nuclei or any major ongoing mergers, though there may be a slight asymmetry present.
