The galaxy presents as a largely smooth, centralized luminosity profile. The light is concentrated in a distinct central bulge region, with a gradual decrease in intensity toward the outer edges. The overall shape is elliptical, appearing relatively circular, with no obvious spiral arm structures or prominent disk features visible. The galaxy exhibits a yellow-orange hue, suggestive of an older stellar population and a lower rate of ongoing star formation. There are no clear indications of tidal disturbances, major mergers, or significant irregularities in its morphology, indicating a relatively undisturbed evolutionary history.
