The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that is yellowish, suggesting an older stellar population dominates the core region. The outer regions show a bluer hue, potentially indicating the presence of younger, hotter stars and ongoing or recent star formation. The galaxy's shape is moderately elongated, appearing more 'in-between' rounded and cigar-shaped. There is no clear evidence of spiral arms or a well-defined disk structure. No major mergers or significant tidal disturbances are readily apparent in the image, though some minor irregularities cannot be ruled out based on the resolution. The light is relatively consistent across the galaxy; there do not appear to be any major areas of intense emission.
