The galaxy presents a somewhat elliptical morphology, appearing relatively smooth in structure. The color profile suggests a dominant older stellar population, evidenced by its reddish-yellow hue. There is a subtle asymmetry, with a slight elongation indicative of a disc-like structure viewed at an angle. No distinct spiral arms or prominent dust lanes are discernible within the limits of resolution. Indications of weak star formation are visible, but likely in a relatively low amount. The general shape is more in the form of a rounded cigar, being much longer than it is wide. There is no evidence of ongoing major mergers or significant tidal disturbances from nearby galaxies.