The galaxy presents as a moderately luminous object with a discernible structure. Its overall morphology appears to be relatively smooth, with a slight ellipticity. There is a suggestion of a diffuse stellar halo extending beyond the main galactic body. The galaxy's color profile indicates a relatively evolved stellar population, with a dominant redder hue and hints of more recent star formation in the form of some bluer regions. There appears to be little evidence of major tidal disturbances or ongoing mergers, although subtle asymmetries might suggest minor gravitational interactions in its past. The half-light radius appears to be a few kiloparsecs. Although its stellar mass appears high, its star formation activity is quite low.
