The galaxy presents as a relatively smooth, elliptical morphology, with a concentrated central bulge that dominates its overall structure. The light distribution indicates a spheroid shape, appearing more round than elongated. There is a gradual decline in luminosity from the core outward. A slight color gradient exists; the central region exhibits a yellowish hue, suggesting an older stellar population, whereas the outer regions seem marginally bluer, implying some presence of younger stars, however a lack of spiral arms or obvious star forming regions makes these differences subtle. No evidence of significant dust lanes, tidal tails, or ongoing mergers is apparent. The galaxy appears undisturbed, lacking any prominent features indicative of recent major interactions.
