The galaxy appears to be a member of a small group, possibly interacting with two other nearby galaxies. The subject galaxy itself exhibits a generally smooth morphology. There is some indication of a faint disk-like structure, though it is not sharply defined. It is relatively compact with a moderate size. The central region appears relatively smooth and is yellowish, with some evidence of star formation. The observed color index suggests ongoing, but moderate star formation activity. Overall, the galaxy is likely an intermediate mass system. There are some indications of minor disturbances possibly due to past or ongoing interactions with other galaxies in the group. A small fraction of the light is associated with brighter, potentially younger stellar populations. The morphology suggests the system may be in the process of transitioning from a spiral-like or irregular structure towards a more spheroidal configuration.
