The galaxy appears as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades towards the outer regions. There is a subtle elongation, suggesting a possible deviation from a perfectly spherical shape. Color gradients are present, with the central region exhibiting a yellowish hue, possibly indicative of an older stellar population. The outer regions show hints of bluer colors, potentially signifying younger stars, or a lower level of active star formation. There's no immediately apparent evidence of a significant disk component, spiral arms, or major disturbances from mergers, although there may be minor irregularities. The overall structure suggests a galaxy in the process of, or already having undergone, morphological transformation toward a spheroidal system.
