The galaxy presents as a flattened spheroid, exhibiting a smooth, diffuse morphology. The color distribution suggests a dominant stellar population in the central region, which appears to be a more yellow or golden hue indicating older stars. The outer regions display a slightly bluer tint, possibly indicative of younger stellar populations or ongoing star formation, although star formation is not significant. The disk is not perfectly round, appearing somewhat elongated or cigar-shaped. There is no strong evidence of tidal tails or significant disturbances, although there is minor asymmetry suggesting possible interactions or disturbances. The galaxy does not appear to be undergoing a major merger.
