The galaxy appears to be a relatively smooth, elliptical-like structure. It presents with a bright, concentrated central bulge that dominates the overall luminosity. There is no apparent spiral arm structure or significant dust lane obscuration visible. The light gradually fades outwards from the core. The color profile suggests a possible redder hue in the outer regions as compared to the central region, which may be indicative of older stellar populations or a lower star formation rate in the outskirts. The galaxy appears to be mostly undisturbed, with no obvious signs of recent major merger events.
