The galaxy presents as a single, luminous object with a primarily smooth morphology. It exhibits a centrally concentrated luminosity profile, with light intensity decreasing radially outwards. The isophotes appear generally elliptical. There may be evidence of a very subtle disk-like structure, though the smoothness of the overall appearance makes it difficult to confirm. The galaxy is reddish in color suggesting an older stellar population. There are no obvious signs of spiral arms, active star formation, or major disturbances indicative of recent mergers, although minor tidal features or interactions cannot be entirely ruled out given the image resolution. The galaxy's overall structure is consistent with that of an early-type galaxy, potentially an elliptical or lenticular system.
