The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is approximately round, with minimal elongation or asymmetry visually apparent. The galaxy exhibits a color gradient, transitioning from a bluer hue in the central regions to a redder tone in the outer parts. There is no evidence of spiral arms or a distinct disk structure. No obvious signs of recent or ongoing major merger events are noted, though there might be subtle disturbances in the outer isophotes suggestive of minor interactions. The galaxy's overall appearance indicates an evolved system, likely dominated by an older stellar population.
