The galaxy presents as a relatively smooth, elliptical structure. The light is centrally concentrated with a bright core and a gradual decrease in luminosity outward. There is a slight elongation, but overall the shape is mostly round. No distinct spiral arms or prominent dust lanes are visible in the image. The galaxy displays a subtle blue hue in its outer regions, hinting at the presence of some young, hot stars, though the overall color suggests an older stellar population. There is no evidence of any major tidal disturbances or ongoing mergers. The overall morphology indicates a galaxy that is likely to be an early-type system undergoing relatively little star formation.