The galaxy presents as a somewhat elongated structure, with a high degree of apparent smoothness. It exhibits a pronounced cigar shape. The central region appears brighter and more concentrated, fading towards the edges. There is a hint of a possible minor disturbance or tidal feature, though it could also be a smaller galaxy in proximity. The color is predominantly yellowish-orange, which indicates an older stellar population, with a subdued area of red near what appears to be the core or nucleus. The morphology suggests it may be an elliptical galaxy, although a highly inclined spiral disk is also a possible classification. There is no strong evidence of active star formation within the body of the galaxy.