The galaxy appears as a centrally concentrated, smooth object, with an elliptical morphology. The light is dominated by a bluish-white hue in the central region, suggesting a population of relatively young stars. The galaxy's outer regions exhibit a slightly redder color, perhaps indicative of an older stellar population, and decreased recent star formation. There is no clear evidence of spiral arms, bars, or significant dust lanes. A slight asymmetry is detected, potentially indicating a minor interaction or disturbance. The overall visual impression is that of a relatively undisturbed system with ongoing, but likely subdued, star formation.
