The galaxy presents a predominantly smooth morphology, with a distinct central bulge region exhibiting high luminosity. The overall shape approximates a flattened spheroid, appearing more lenticular than spiral. Evidence for a disk component exists, though it is faint and not clearly resolved into spiral arms. There is a slight ellipticity to the overall structure. The color profile suggests an older stellar population, with a redder hue overall. While the primary body of the galaxy appears undisturbed, a faint region exists near the center, possibly indicating minor gravitational interaction, or star formation. The galaxy shows a generally homogenous texture, lacking pronounced knots of star formation or dust lanes. It appears relatively massive with a low rate of current star formation. The light is concentrated centrally, indicating it may be an early type galaxy.
