The galaxy presents as a single, largely homogenous structure with a smooth, somewhat elliptical morphology. There is no immediately apparent disk or spiral arm structure. The light profile suggests a centrally concentrated luminosity gradient, with a bright core gradually fading towards the outer regions. Color distribution appears generally uniform with an overall yellowish or golden hue. The structure appears undisturbed with no signs of major mergers or tidal disruptions evident in this imaging. Slight elongation is seen in one direction, but the overall form is close to circular. Based on these observations, the galaxy is likely a massive elliptical galaxy.
