The galaxy presents an overall elliptical morphology, with a smooth appearance to its light distribution, suggesting a relatively evolved stellar population. The galaxy's color gradient indicates a redder core region, potentially indicative of older stars and/or dust obscuration towards the center.  There is a hint of a disk structure, though the dominant feature is spheroidal. No strong evidence of spiral arms is discernible. There might be a very minor disturbance or interaction occurring.
