The galaxy presents an elliptical morphology, appearing somewhat elongated in shape. It exhibits a smooth, relatively featureless structure, lacking prominent spiral arms or distinct dust lanes. The central region of the galaxy displays a higher concentration of light, indicative of a bulge. The overall color profile leans toward the redder end of the spectrum, suggesting a population of older stars and a lower rate of active star formation. There is a subtle color gradient, with the central bulge appearing slightly more yellow/orange than the outer regions, which fade into a dimmer, redder halo. There is no apparent interaction with neighboring galaxies or evidence of recent merger activity based on visible tidal features or distortions.
