The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that dominates the overall luminosity. The light distribution appears highly symmetrical, with a gradual decrease in intensity from the core outward. There is no apparent spiral arm structure or significant dust lane obscuration visible. The color profile suggests an older stellar population, likely consisting primarily of evolved stars, particularly towards the core region. A faint, extended halo surrounds the brighter central region. There is no evidence of major tidal disturbances or ongoing merger activity. Overall, the galaxy appears to be a relatively quiescent, early-type system.
