The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright core, indicative of a high stellar density. Moving outwards from the core, the luminosity gradually decreases, with a smooth transition into the fainter outer regions. There's a slight elongation of the galaxy shape with it appearing to have a cigar shape. The color profile suggests a generally older stellar population, with a redder hue dominating the central bulge. Fainter blue features or patches can be observed in the outskirts, perhaps suggesting younger populations of stars or some active star formation occurring, albeit at a low level. There is no strong evidence of spiral arms, bars, or other distinct features typically associated with disk galaxies. No major signs of interactions or mergers are immediately apparent, though some minor disturbances cannot be entirely ruled out.
