The galaxy presents as a generally smooth, single structure, possessing a concentrated central region that may be indicative of a bulge. Its overall shape appears somewhat round, though not perfectly circular. There is a marginal hint of subtle disturbances or asymmetries in its outer regions but lacks a defined spiral arm structure. The light emanating from the galaxy is predominantly redder in color, with a hint of yellow. This suggests an older stellar population, and possibly lower rates of ongoing star formation. There may be some minor indications of tidal disturbances, but is not undergoing a major merger.
