The galaxy exhibits a predominantly smooth morphology. Its overall shape appears relatively round. There is a subtle but noticeable color gradient, shifting from a bluer hue at the center to redder tones in the outer regions. Evidence of merging is largely absent, though there may be slight visual irregularities indicative of a minor disturbance. The galaxy's light is somewhat concentrated toward the core, exhibiting a gradual decline in surface brightness with increasing radius. There are no distinctly resolved features such as spiral arms or a prominent central bar visible in this image.
