The galaxy presents as a singular, somewhat indistinct, luminous object with a diffuse morphology. The light profile appears to be centrally concentrated but lacks a well-defined structure, hinting at a smooth distribution of light.

There is a suggestion of spiral arm structures, though they are faint and not clearly delineated. Overall, the galaxy has a notable red color, which may imply a relatively old stellar population and a lower rate of star formation, though some regions appear to have pockets of more recent star formation.

There are areas in the galaxy that indicate disturbances to the morphological structure; this may suggest interactions with another galaxy, or merging event. 
