The galaxy appears to be a smooth, elliptical system. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo. The color profile suggests a relatively old stellar population, with a yellow-red hue dominating the central region. The galaxy is elongated, exhibiting a cigar shape rather than appearing circular. There are no apparent signs of ongoing major mergers or significant tidal disturbances in this image, with only minor disturbances possible. The light distribution indicates a centrally concentrated mass profile, consistent with a massive elliptical galaxy.
