The galaxy presents a generally smooth morphology, with a shape that appears mostly round, although there is a slight elongation. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a galactic bulge. There is subtle variation in the color across the galaxy, with a possible tendency towards redder hues in the center, indicative of an older stellar population, with more green/blue hues on the outside, indicating a young star population. Evidence of possible tidal disturbances or ongoing mergers may be visible.
