The galaxy presents as a spiral type, although the inclination obscures a clear view of the disk structure. There appears to be a substantial central bulge, with a moderate level of brightness. Two prominent spiral arms emerge from the central region, exhibiting a moderately wound structure. Traces of a bar feature may be present, subtly elongating the central bulge, although the structure is not overtly prominent. The overall disk color appears bluer than the central bulge. Signs of minor disturbances, such as slight asymmetries or distortions in the spiral arms, are present.
