The galaxy presents a largely elliptical morphology, exhibiting a smooth light distribution. The color profile appears generally uniform across the visible structure. There is a lack of strong spiral arm features or prominent dust lanes. The galaxy shows a high degree of central concentration, with a bright core that gradually fades into the outer regions. There is no obvious presence of ongoing major mergers or tidal disturbances, though there is a slight asymmetry in the light distribution, suggesting a possible minor interaction in the galaxy’s past.
