The galaxy presents as a single, relatively smooth, roundish entity. The light profile appears centrally concentrated, with the core exhibiting a yellowish hue. This color likely indicates an older stellar population. Fainter, bluer light surrounds the central region, potentially signifying the presence of younger stars in the outer areas. Overall, the galaxy appears fairly undisturbed, with no obvious signs of major mergers or tidal disruptions. There might be some minor irregularities in the outer edges, which could indicate a minor disturbance or some ongoing accretion.
