The galaxy presents as a somewhat diffuse object with a relatively smooth overall structure. It appears to have a subtle disk-like morphology, although not sharply defined. There is some indication of a disturbance or faint feature extending from the main body of the galaxy, possibly a tidal tail or an interacting companion galaxy. A merging event cannot be ruled out, though the features are not highly pronounced. The galaxy appears to be brighter in the green and red bands, indicating a possible mix of stellar populations, including both older, redder stars and younger, bluer stars. The galaxy’s center is slightly brighter than the rest, although there is no clear bulge. Its size is moderate; it occupies a few arcseconds on the sky.
