The galaxy presents as a luminous, relatively compact object exhibiting a smooth, elliptical morphology. There is a slight elongation, but not a significant deviation from a circular shape. The core is a bright, diffuse central bulge dominating the overall light profile. The color appears to be a yellow-orange hue, suggestive of an older stellar population with minimal ongoing star formation activity. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances. There is a hint of a weak disk, but the overall structure is dominated by the spheroidal component.
