The galaxy presents as a singular, moderately luminous object with a significant degree of spatial extent. The overall morphology appears to be elliptical or spheroidal, exhibiting a generally smooth light distribution. There is an indication of a slightly irregular shape and some evidence of internal structure, possibly suggesting ongoing or recent interaction or merging activity. The color profile indicates the galaxy has experienced active star formation. The core is quite bright, hinting at the possibility of an active galactic nucleus (AGN) but further investigation would be required to verify its existence. There are indications of minor disturbances and some potential merger remnants. These might suggest tidal tails or bridges, although high-resolution imaging would be necessary for confirmation.
