The galaxy presents as a moderately small, somewhat amorphous structure. The overall color appears bluish, suggesting the presence of younger, hotter stars. There is a brighter central region indicating a possible core or bulge. While the galaxy doesn't exhibit strong spiral arm structures, there are some faint irregularities and hints of a disk-like component. There is also some indication of a possible minor disturbance or interaction, though no obvious tidal tails or bridges are visible. The rate of star formation appears to be relatively low.
