The galaxy presents as a moderately bright, elliptical or lenticular structure, exhibiting a smooth, largely featureless morphology. The light distribution suggests a significant bulge component, centrally concentrated, with a gradual decrease in luminosity outwards.  There is a hint of bluer color in some of the outer regions, potentially indicating some ongoing, albeit subdued, star formation, though the overall color profile seems consistent with an older stellar population. The shape appears mostly regular, without strong evidence of tidal features or major disturbances, although a slight asymmetry cannot be entirely ruled out. This galaxy has a likely stellar mass around 10^9 solar masses, and a low star formation rate. The size is relatively compact, around 4 kpc across.
