The galaxy presents as an elongated, cigar-shaped structure, suggesting it is likely an elliptical or lenticular galaxy viewed at an angle. It exhibits a prominent central bulge that gradually fades into a diffuse halo. The core appears to be a mix of yellow and white light, with what looks like a slight amount of blue on the edge of the core. There is an indication of a faint, extended disk or arm feature on the opposite side of the core. The galaxy appears relatively undisturbed with no significant signs of tidal interactions or ongoing major mergers. The smooth light distribution and lack of strong spiral arm structures or prominent dust lanes suggest a relatively low star formation rate within the central region.
