The galaxy exhibits a generally smooth morphology, with a central, luminous bulge. The light distribution appears relatively even, indicating a lack of significant spiral arm structure or prominent dust lanes. The overall shape is approximately circular, suggesting a classification towards elliptical or lenticular. The color gradient transitions from a more yellow-orange hue in the core to a bluer tint in the outer regions, suggesting a shift from older stellar populations in the center to younger populations toward the periphery. No strong evidence of tidal features or ongoing major mergers are apparent, although some subtle irregularities might indicate minor disturbances or past interactions. Overall, the galaxy presents as a relatively evolved system.