The galaxy presents a generally smooth, elliptical morphology, exhibiting a centrally concentrated luminosity profile that decreases gradually outwards. It appears largely featureless, with no readily discernible spiral arms or prominent dust lanes. The core region presents a yellowish hue, which may indicate an older stellar population dominated by redder stars. The outer regions transition to a slightly bluer tint, suggesting the presence of some younger, hotter stars. The overall roundness is a prominent aspect, with only a slight deviation from a perfect circular shape. There is no obvious indication of major mergers or significant tidal disturbances affecting the galaxy's structure, although minor disturbances cannot be entirely ruled out given the image resolution.
