The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The light profile appears relatively symmetrical, lacking any prominent spiral arm structures or significant irregular features. The color is predominantly yellowish-orange, suggesting a stellar population dominated by older, redder stars. The lack of strong blue emission indicates a low rate of ongoing star formation. There is a slight elongation in its shape, deviating marginally from a perfect sphere. Overall, the galaxy appears to be a relatively quiescent system with little signs of recent interactions or mergers.
