The galaxy appears as a centrally concentrated object with a bright, unresolved core. There is faint, diffuse emission extending outwards from the core, suggestive of a disk or halo-like structure. The color profile indicates a bluer hue in the central regions, possibly indicating younger stellar populations or active galactic nucleus activity. There is evidence of a minor disturbance or tidal feature in the form of an extension on both the left and right sides, perpendicular to the plane of the object. The object displays a relatively high degree of smoothness, with no apparent spiral arm structures or significant dust lanes visible at this resolution. The faint and fuzzy surrounding emissions could also indicate a possible merger event.
