The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile, suggestive of an older stellar population. There are no obvious spiral arm structures or dust lanes visible, but the presence of bluer colors on the edge of the galaxy suggests some low-level ongoing star formation. The galaxy displays a moderately elliptical shape, being neither perfectly spherical nor highly elongated. There's no strong indication of tidal disturbances or ongoing major mergers, though some subtle asymmetry cannot be completely ruled out. It is relatively bright, indicative of a high luminosity, likely corresponding to a substantial stellar mass.
