The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The light profile suggests a relatively old stellar population, with a yellow-red hue dominating the visual spectrum. The absence of distinct spiral arms or significant dust lanes indicates a lack of ongoing, large-scale star formation. A subtle extension of light suggests the presence of a faint halo or tidal features, possibly indicative of past minor interactions or accretion events. Overall, the galaxy exhibits a morphology consistent with an evolved system approaching quiescence.
