The galaxy appears as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a slight elongation visible, but overall it presents a rounded appearance. The galaxy's light is primarily concentrated in the central region, with a gradual fading towards the outer edges. There is little evidence of significant spiral arm structure or prominent dust lanes. Minor disturbances cannot be excluded due to resolution limitations, but the overall appearance suggests a system that is either undisturbed or in a late stage of merging. The color profile indicates the presence of older stellar populations, suggesting a low rate of current star formation within the galaxy.
