The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a high density of stars. The light profile gradually decreases outwards from the core, fading into the background sky. There is a subtle elongation, suggesting a deviation from a perfect spherical shape, leaning slightly towards a more flattened ellipsoid. The color appears to be relatively uniform across the galaxy, with a yellow-orange hue, suggestive of an older stellar population and relatively low levels of ongoing star formation. There appears to be a slight asymmetry in the outer regions, potentially indicating a minor gravitational interaction or past merger event that may have disturbed the galaxy's structure. Overall, the galaxy appears to be a massive system.
