The galaxy presents as a somewhat elliptical, face-on system. There is a bright central bulge that dominates the luminosity profile, exhibiting a concentrated, yellowish-white color. The outer regions of the galaxy display a bluer hue, indicating the presence of younger stellar populations and ongoing star formation, albeit at a modest rate. 

There is a noticeable disturbance or asymmetry in the galaxy's morphology, possibly indicative of a minor interaction or recent merger event. This is further suggested by subtle distortions within the galactic disk.

Overall, the galaxy appears to be an intermediate-mass system, potentially transitioning from a more actively star-forming state to a more quiescent elliptical morphology.
