The galaxy presents as a somewhat asymmetrical, moderately luminous object with a smooth overall appearance. The central region exhibits a concentrated, brighter core, possibly indicative of an older stellar population. Extending outward from the core, a fainter, more diffuse disk-like structure is observed. There is a very subtle hint of blue color in the outer regions of the disk, possibly indicating a small amount of ongoing star formation. Based on its apparent ellipticity, the galaxy's disk is inclined relative to our line of sight. There are no obvious signs of strong tidal disturbances or interactions with neighboring galaxies, although a slight asymmetry in the outer disk region suggests the possibility of a minor past interaction. The galaxy’s redshift indicates a relatively low distance, implying a dwarf type galaxy.
