The galaxy presents as a relatively well-defined, flattened, and elongated structure. The central region exhibits a notable concentration of luminosity, appearing bright and smooth, possibly indicative of an older stellar population. Moving outwards from the center, the galaxy displays a gradual decline in surface brightness. 

There is evidence of a disk-like morphology although the galaxy is more rounded than a typical disk galaxy. The overall color suggests it may be an intermediate-type galaxy, between a spiral and an elliptical. Hints of bluer regions may indicate recent or ongoing star formation, even if at a low rate. There appear to be no major signs of tidal disturbances or mergers.
