The galaxy presents as a disk galaxy, likely seen at a moderately inclined angle relative to our line of sight, appearing somewhat cigar shaped. The central bulge is prominent and appears relatively smooth and featureless, with a concentrated brightness. The disk component exhibits a smoother texture overall, with a slight hint of spiral arm structure. There may be some minor tidal disturbances, but the bulk of the galaxy is relatively undisturbed. The color gradient suggests a population of older stars dominating the bulge, with hints of younger stellar populations present in the disk. The galaxy has a smooth overall appearance, with no major mergers occurring.
