The galaxy presents a relatively smooth morphology, yet is not perfectly elliptical. It exhibits a discernible disk-like structure, though it is not strongly defined. The color distribution suggests ongoing star formation, particularly in a ring-like region encompassing the central bulge. A slight elongation is visible, classifying it as tending to be "cigar" shaped. There are no strong visual indications of major mergers or significant tidal disturbances, suggesting a relatively isolated and undisturbed system.
