The galaxy presents a generally smooth and rounded morphology. Its light profile appears centrally concentrated, exhibiting a gradual decrease in surface brightness from the core outwards. The overall color is slightly red-shifted, hinting at an older stellar population. There is no clear evidence of spiral arms, a bar, or any signs of ongoing major merging activity. Subtle irregularities or minor disturbances may exist in the outer regions, but they are not a prominent feature. The galaxy is relatively compact in size.
