The galaxy appears to be a relatively compact, though not entirely smooth object. It exhibits a disk-like structure but it is not strongly defined. There is only slight suggestion of spiral arms or other distinct features.

The galaxy's color profile is generally red, with hints of green or yellow. This suggests that the galaxy is comprised of an older stellar population, potentially indicating a higher proportion of evolved stars and a reduced rate of star formation.

Based on the small disturbances within the galaxy, it can be deduced that this galaxy is likely undergoing or has recently undergone a minor merger or interaction with another smaller galaxy. There is a hint of an asymmetry in the galaxy's shape which supports this interaction.
