The galaxy presents as a luminous, extended structure with a generally elliptical morphology. A smooth central bulge dominates the overall light distribution, exhibiting a yellowish hue, potentially indicating a population of older stars. Extending outwards from the core are fainter, diffuse regions with hints of bluer colors, possibly associated with ongoing star formation. The overall structure shows subtle irregularities, suggesting minor gravitational interactions or disturbances in the recent past. There are no clear signs of a prominent disk or spiral arms. The galaxy appears relatively isolated, although there are neighboring objects within the field of view.
