The galaxy presents a generally smooth and rounded morphology. Its light profile appears centrally concentrated, suggesting a dominant spheroid component. There are no obvious spiral arm structures or a prominent disk visible. The color is somewhat uniform across the galaxy, with a tendency towards the redder part of the spectrum, indicative of an older stellar population and/or dust obscuration. There are no clear signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity. There is a small green section towards the middle of the galaxy, which could be a result of a recent star forming event, though it is difficult to discern from the surrounding dust. Overall, the galaxy exhibits characteristics consistent with a massive, relatively quiescent system.
