The galaxy presents as a slightly elliptical, disk-like structure. Its core exhibits a bright, concentrated luminosity, suggestive of a substantial stellar population or possibly AGN activity, though the resolution limits definitive assessment. The central region displays a yellowish-white hue, possibly indicating an older stellar population dominating the region. The outer disk appears more diffuse. There is a slight hint of bluer regions within the disk, suggesting the presence of younger, hotter stars and star-forming regions. There is a slight disturbance on one side, perhaps indicative of a minor interaction. Overall, the galaxy seems to be relatively undisturbed, showing no significant signs of ongoing major mergers or tidal disruptions.
