The galaxy presents as a relatively compact, elliptical system. The core exhibits a bright, concentrated intensity, suggesting a high stellar density or active galactic nucleus. The light profile appears smooth and diffuse, transitioning gradually from the central bulge outwards. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy's color is predominantly yellow, indicative of an older stellar population with a low star formation rate. The overall morphology is well-defined, with no signs of significant tidal disturbances or ongoing major mergers. There is a slight asymmetry in the outer regions, hinting at a possible minor interaction in the past. The shape approximates a circular profile, with minimal elongation.
