The galaxy presents as a mostly smooth, lenticular or elliptical structure, with a significant central bulge. The morphology is largely spheroidal, but demonstrates a slight elongation, trending towards a cigar shape. The central region exhibits a yellowish hue, potentially indicating an older stellar population and/or dust obscuration. Moving outward from the center, the galaxy's color shifts to a bluer tint, suggesting the presence of younger stars, and potentially areas of active star formation in the outer regions. Faint, diffuse extensions are observed at the edges of the galaxy, particularly at the end of the cigar-shaped structure. These extensions could be tidal features indicative of past or ongoing gravitational interactions. The overall structure suggests a relatively evolved system, but there are hints of ongoing activity or recent disturbances. The central region is notably brighter compared to the outer disk.