The galaxy presents as a lenticular or early-type spiral, exhibiting a primarily smooth morphology. The central bulge is prominent and appears largely spheroidal, with a yellowish hue suggesting an older stellar population. A faint, disklike structure extends from the bulge, elongated in shape, but with minimal discernible spiral arm features. The disk displays a bluer color gradient moving outward from the bulge, indicating some level of ongoing star formation, albeit at a low rate. The galaxy shows a slight degree of asymmetry, possibly suggesting a previous minor interaction. There is no evidence of a major merger event or significant tidal disturbances in the surrounding vicinity of the galaxy.
