The galaxy presents as a moderately bright, elliptical-shaped object. Its color profile appears somewhat blue-white, indicative of a likely population of younger, hotter stars. The galaxy's light distribution shows a centrally concentrated bright nucleus, gradually decreasing in intensity towards the outer edges. A slight elongation is apparent, with the morphology leaning towards a "football" or cigar-shaped profile rather than a perfect sphere. There is some visible asymmetry or perturbation in the outer regions, possibly suggesting minor tidal interactions or ongoing mergers. The galaxy exhibits a smooth appearance, with no obvious spiral arms or significant dust lanes visible. The overall structure does not suggest a heavily disturbed morphology, although subtle features point to some level of interaction.
