The galaxy appears as a diffuse object, elongated and somewhat faint. Its color profile suggests a redder hue, possibly indicative of an older stellar population or significant dust obscuration. There are no clear spiral arm structures or a prominent central bulge visible; instead, its luminosity is distributed relatively evenly across its structure. Irregularities in the light distribution hint at possible disturbances or interactions. There is a very faint tail-like feature extending outward from the main body, suggestive of tidal interactions or past merger events.
