The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. There is a concentrated central bulge that dominates the overall light profile. Fainter, diffuse light extends outwards from the bulge, suggesting a more extended halo. The color gradient shows a subtle trend, appearing bluer towards the outer regions and redder within the bulge, potentially indicating older stellar populations concentrated centrally. The galaxy appears relatively isolated with some possible indication of a minor tidal interaction or disturbance at one side, although this is not clear.
