The galaxy presents a largely smooth, elliptical morphology. The central region displays a bright, concentrated core which decreases in surface brightness outwards. There appears to be a slight extension that gives it an oblate shape. The color profile is suggestive of an older stellar population, exhibiting a yellowish-white hue in the core region. The outskirts show a bluer tint, with a slight hint of ongoing star formation. There are no obvious signs of spiral arms or a prominent disk structure. The galaxy seems relatively undisturbed, lacking any major signs of tidal interactions or mergers, although a very slight asymmetry in its outer edges may indicate some past minor gravitational interactions.
