The galaxy appears as a somewhat diffuse, reddish-orange object, suggesting an older stellar population or significant dust obscuration. Its morphology seems disturbed, possibly exhibiting signs of tidal interactions or ongoing merger activity. There might be a faint disk or ring-like structure present. A notable feature is the presence of a central, slightly more concentrated region, hinting at a possible bulge or nucleus. There's a slight elongation visible. The galaxy lacks a well-defined spiral arm structure.
