The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent and exhibits a bright, concentrated luminosity. The galaxy's overall shape is moderately elongated, appearing somewhat cigar-shaped rather than perfectly spherical. There is a hint of a disk-like structure extending from the central bulge, but it is not clearly defined or highly structured. Evidence for spiral arms or significant dust lanes is absent. There are no obvious signs of recent major mergers or significant tidal disturbances, although minor irregularities cannot be ruled out. The color gradient appears to be redder in the central regions, potentially indicating an older stellar population with less ongoing star formation. The outer regions show a bluer hue, which can be indicative of some younger stars, but the relative lack of blue light and the presence of light across all bandwidths shows a lack of very significant star formation. Overall, the galaxy appears to be an evolved system, likely a relatively massive elliptical or lenticular galaxy with a history of limited recent star formation.
