The galaxy presents as an elongated, distorted structure, possibly indicative of an edge-on spiral or lenticular type. The central region exhibits a concentrated luminosity, with a yellowish-white hue, suggesting an older stellar population or significant dust obscuration. Extending from the core are faint, diffuse extensions that exhibit a bluer tint, which may indicate younger stars and ongoing star formation. The overall shape of the galaxy shows a degree of asymmetry, possibly due to gravitational interactions or recent merger activity. A slight warp is present in the main disk structure of the galaxy.
