The galaxy presents as a lenticular or early-type spiral galaxy. It exhibits a somewhat elongated morphology, with an apparent major axis extending roughly northwest to southeast. A notable feature is the presence of a bright central bulge, which appears slightly yellowish, indicative of an older stellar population. The disk component shows a bluer hue. This suggests the presence of some on-going, albeit potentially weak, star formation, concentrated within the disk. The overall structure appears relatively smooth and undisturbed, with no immediately obvious signs of tidal interactions or major merging events. The galaxy displays a moderate degree of inclination relative to our line of sight. This inclination obscures any potential spiral arm structure, making a precise morphological classification challenging based solely on visual inspection.
