The galaxy presents a somewhat elliptical morphology, exhibiting a diffuse, luminous core.  The light distribution indicates a relatively smooth structure.  The color gradient suggests a population of older stars, potentially dominating the overall light emission. There appears to be a hint of a disk-like structure, but the dominant feature is the smooth, centrally concentrated bulge.  There is a slight asymmetry visible, with minor disturbances observed in the outer regions, possibly suggestive of an interaction. No prominent spiral arms or well-defined star-forming regions are discernible at this resolution.
