The galaxy presents as a lenticular or early-type spiral galaxy, viewed at a moderate angle close to edge-on. The light distribution suggests a dominant spheroid component with a smooth, centrally concentrated bulge exhibiting a yellowish-white hue, which could be indicative of an older stellar population. Fainter disk-like structures extend outwards from the bulge, displaying a bluer tint, possibly indicating the presence of some younger stars or regions of ongoing star formation. No distinct spiral arm structures or prominent dust lanes are discernible within the disk. The galaxy appears relatively undisturbed, showing no clear signs of recent major mergers or tidal interactions. Overall, the galaxy appears to be a quiescent system with a moderate stellar mass and relatively low ongoing star formation activity. The size appears to be relatively small.
