The galaxy presents as a lenticular, disk-shaped structure with an apparent cigar-like ellipticity. The central bulge region exhibits a relatively smooth, concentrated profile with a yellowish-orange hue, suggestive of an older stellar population and less active star formation. Fainter disk components extend outwards from the bulge. These show a bluer color profile, indicating younger stars and ongoing star formation within these outer regions. There is no clear indication of a spiral arm structure. Evident color gradients between the central bulge and the outer disk suggest spatial variations in stellar population ages and metallicities. No major signs of interaction or merging are visible, although slight disturbances could be present, meriting further investigation.
