The galaxy presents as a generally smooth object with an elliptical morphology. It exhibits a relatively concentrated luminosity profile with a prominent central bulge. The color gradient is subtle, showing a slightly redder core transitioning to a bluer outer halo. There is no evidence of distinct spiral arms or a pronounced disk structure. The overall appearance suggests an evolved system with potentially low levels of recent or ongoing star formation. No major interactions or tidal features are immediately apparent, though subtle disturbances cannot be entirely ruled out. The galaxy's round shape indicates that it is not a late stage merger. A slight asymmetry is present and may indicate a possible minor interaction.
