The galaxy presents as a relatively smooth, elliptical object. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades outwards into a less luminous, greenish halo. The overall shape is elongated, approaching a cigar-like morphology, but is predominately in between round and a cigar shape. There is no clear evidence of spiral arms or significant dust lanes. Subtle disturbances in the galaxy's outer regions suggest possible minor interactions or past mergers. The galaxy exhibits a blue-ish green hue in its outer regions, potentially indicating ongoing star formation, albeit at a relatively low rate.
