The galaxy presents a moderately elliptical morphology, appearing as a diffuse, centrally concentrated object. The light distribution transitions smoothly from the core outwards, showing no distinct spiral arm structures or bar features. A notable color gradient is apparent, with a yellowish-white hue dominating the central region, suggestive of an older stellar population. Moving outwards from the core, a subtle shift towards bluer tones is observed in the outer regions, potentially indicating the presence of younger, hotter stars. The overall smoothness of the light profile points toward a relatively relaxed system. There are no indications of strong tidal interactions or recent major mergers, though subtle asymmetries or faint distortions in the outer regions cannot be entirely ruled out based on this image alone. Overall, the galaxy appears to be a reasonably evolved system, possibly an early-type spiral or a lenticular galaxy seen at a significant distance.
