The galaxy presents as a generally smooth elliptical or lenticular form, appearing elongated with a cigar-shaped morphology. The central region exhibits a concentrated, bright bulge, with a noticeable color gradient indicating a higher concentration of older stellar populations. The outer regions are less defined, fading gradually into the background with a hint of a flattened disk-like structure. No distinct spiral arms or prominent dust lanes are visible, supporting the classification of an early-type galaxy, potentially with on-going but low-level star formation activity. There are no indications of major merger events, though a minor gravitational interaction cannot be fully ruled out based solely on visual inspection.
