The galaxy presents as a centrally concentrated object with a smooth light distribution. Its overall morphology appears elliptical, with a moderate degree of roundness. There is no discernible spiral arm structure or bar. The light profile is dominated by a bulge-like component, lacking significant features indicative of active star formation regions. A faint, extended halo may be present, though difficult to distinguish from background noise. The primary color appears slightly red, suggesting a population of older stars. There is some evidence of a minor disturbance, possibly a small tidal interaction, but overall, the galaxy appears relatively undisturbed.
