The galaxy appears as a concentrated, centrally-brightened object. It displays a largely smooth morphology, showing little evidence of spiral arms or significant substructure. The radial light profile suggests a gradual decline in brightness from the center outwards, implying a centrally dominant stellar population. The overall shape is nearly circular, with minimal deviation from perfect rotational symmetry. There may be faint indications of a slightly extended halo, but this is not definitively resolved. The color gradients are subtle; the central region presents a yellowish-white hue which possibly transitions to a redder color in the outskirts, suggesting that the galaxy's outskirts are populated by older stars. No major interactions or tidal features are obvious. Based on the available information, the galaxy most likely represents an elliptical or an S0-type galaxy viewed at a significant distance.
