The galaxy appears as a centrally concentrated object with a smooth overall morphology. The core region exhibits a bright, somewhat elliptical shape, suggesting a bulge component. The light distribution fades gradually outwards from the core, with a more diffuse and less structured envelope surrounding the central region. There's a slight elongation to the galaxy's shape, more in an "in between" shape than extremely cigar shaped. The overall color profile indicates a predominantly older stellar population, with a tendency towards redder hues emanating from the central bulge. Possible slight disturbances in the outer regions, but overall shape is mostly undisturbed.
