The galaxy presents as a relatively smooth, rounded structure. The light profile appears centrally concentrated, with a gradual falloff in intensity moving outwards from the core. The color gradient transitions from a yellowish-white in the central region to a slightly redder hue in the outer regions.  There is no readily apparent disk structure or spiral arm morphology.  Subtle asymmetries or minor disturbances may be present in the outer regions, but the resolution limits detailed morphological classification.  The overall structure is indicative of an early-type galaxy with a significant spheroidal component. The central region displays a relatively high surface brightness, indicating a dense stellar population. Star formation appears low.
