The galaxy presents as a relatively smooth, centrally concentrated object, with a morphology appearing largely spheroidal. The galaxy exhibits a dominant bulge component with a yellowish hue, suggesting a population of older stars. There is a faint, diffuse halo surrounding the central region, extending outwards and fading into the background. The galaxy displays a slight asymmetry, perhaps hinting at minor disturbances or recent accretion events, although no prominent tidal features are readily apparent in this image. There is minimal evidence of active star formation regions or prominent dust lanes. The galaxy appears to be an elliptical or lenticular galaxy, likely with a relatively low star formation rate.
