The galaxy presents as a centrally concentrated spheroid with a generally smooth morphology. The light profile appears to decline radially from a bright, yellowish core. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy exhibits a slight ellipticity, but it is generally round in appearance. Fainter, diffuse light extends outward from the central region, gradually fading into the background. The color gradient suggests an older stellar population dominating the central bulge, with a possible presence of younger stars in the outer regions. There is no strong indication of tidal features or ongoing major mergers, although some minor disturbances cannot be ruled out.
