The observed galaxy presents a somewhat amorphous morphology, suggesting a possible transitional type between elliptical and spiral forms, or a galaxy undergoing interaction. Its overall color appears to be reddish, potentially indicating an older stellar population and reduced current star formation. The distribution of light is relatively smooth, although subtle features hint at the presence of a disk-like structure. There is evidence of a slight central bulge. The galaxy does not exhibit clear spiral arms. The relatively compact size suggests a classification as either a dwarf galaxy or a more distant, larger system. Possible signs of minor tidal disturbances exist. Further spectroscopic analysis is required to determine the exact star formation rate, age, and dynamical state of this galaxy.
