The galaxy presents as a relatively smooth, lenticular structure. Its overall shape is elongated, leaning towards a cigar-shaped morphology. The central bulge appears prominent, exhibiting a color gradient shifting towards redder hues. The disk is barely visible; it is only slightly resolved within the limits of the available data. There is no clear spiral arm structure discernable. There appear to be no significant tidal tails or prominent signs of an ongoing major merger event, although some minor asymmetries hint at possible gravitational interactions. The color profile suggests that it is composed of an older stellar population in the center, with a slight enhancement of younger, bluer stars. The galaxy appears moderately luminous.
