The galaxy presents a disk-like morphology with a central bulge. The disk exhibits subtle features, possibly spiral arm segments or dust lanes, though its structure is not well-defined. There is a general smoothness to its light profile, but some irregularities and asymmetry are present. Some evidence of disturbances, such as minor tidal features, might be present, though the details of the galaxy appear to be poorly resolved. The galaxy has a moderate luminosity and appears relatively isolated, but not in a stage of active merging with any other prominent nearby galaxies. There is a slight color gradient, the central regions appearing slightly redder than the outer disk, possibly indicating an older stellar population in the core. 
