The galaxy appears to be generally smooth in morphology, with a concentrated central bulge. There is evidence of tidal disturbance, where we may be observing a potential ongoing merger with a smaller satellite galaxy or tidal tail. The colour of the central region is yellowish-red, suggesting an older stellar population, while the features are slightly bluer in colour. This could indicate areas of more recent star formation occurring within the disturbance. The overall shape appears mostly rounded. The galaxy may be an early-type galaxy with recent or ongoing interactions.
