The galaxy presents a generally smooth and rounded morphology. There is little to no apparent disk structure. The galaxy exhibits a concentrated central region with a gradual decrease in luminosity towards the outer edges. There is a slight elongation of the galactic structure, deviating from a perfect circular shape. A hint of a possible minor disturbance may be present, though it does not significantly disrupt the overall smooth appearance. The color profile is slightly reddish in hue suggesting an older stellar population. No active star formation regions are readily apparent.
