The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth appearance. The light profile shows a bright core, gradually fading outward. The color gradient suggests that the central region is more reddish than the outer regions. Based on color and the smooth profile, it is likely that the galaxy is composed primarily of older stellar populations. There is no obvious spiral structure or active star formation. A slight elongation is present, indicating that the system is not perfectly spherical. There appears to be no significant interaction or merging activity occurring, with no clear tidal features or morphological disturbances detected in the immediate vicinity. The overall structure indicates a relatively quiescent and evolved system.
