The galaxy presents a largely smooth and rounded appearance, with a notable absence of distinct spiral arms or a bar structure. It appears to be relatively isolated, with no obvious signs of ongoing major mergers or tidal disturbances, though there is an indication of a possible minor disturbance. The color profile suggests a population of older stars, possibly a red elliptical galaxy, but with some indication of ongoing star formation. It presents as a large, massive system. Overall, the galaxy shows characteristics consistent with a mature system.
