The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, concentrated light profile. There is no apparent spiral arm structure or distinct dust lane. The galaxy has a centrally concentrated bulge, surrounded by a diffuse halo of light. The overall shape of the galaxy is round, showing no signs of significant tidal disturbances or elongation. The color is generally yellow, suggesting a population of older stars. Evidence of ongoing or recent star formation is lacking, indicating a relatively passive galaxy. Faint extensions of light emanating away from the central core may be indicative of stellar tidal debris. Based on its appearance, this galaxy is likely a relatively massive system that may be a member of a group of galaxies.