The galaxy presents as a lenticular or possibly early-type spiral system, characterized by a significant bulge component with a relatively smooth, low-contrast spiral arm structure. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. The disk appears elongated, with the major axis oriented horizontally. The galaxy shows a moderate inclination relative to our line of sight. Evidence of ongoing or recent star formation is present, as hinted by bluer regions within the disk, although the overall star formation rate appears relatively low. The object appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a hint of dust absorption along the disk. The galaxy's overall morphology is consistent with a system that has transitioned from a more actively star-forming state to one where star formation is increasingly suppressed.
