The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light profile appears relatively smooth, lacking prominent spiral arms or a distinct bulge. The central region exhibits a high degree of luminosity, suggesting a dense concentration of stars and possibly an active galactic nucleus, although no distinct point source is discernible within the resolution of the image. The isophotes are tightly packed.

A subtle color gradient can be observed, shifting from a slightly bluer hue toward the inner regions to a redder color in the outer halo. This suggests a potential radial gradient in stellar populations, with younger, hotter stars concentrated near the center. Some faint disturbances in the outer regions suggest a past merger or interaction, but nothing significant. 

The overall shape and color distribution is indicative of a lenticular or early-type spiral galaxy, possibly undergoing a transition from a more actively star-forming state to a more quiescent state. However, the presence of some blue light suggests that this galaxy still retains at least a moderate level of ongoing star formation.
