The galaxy exhibits a generally smooth morphology, with an elliptical appearance. The light distribution appears concentrated toward the center, suggesting a large, dense core. While the image quality is limited, there is a slight elongation, but overall the galaxy appears mostly round. There is no obvious spiral structure or significant dust lanes visible. There is also no clear signs of tidal tails or other dramatic distortions, which could indicate recent major mergers. Based on its color, the galaxy looks to be a mixture of older stars and perhaps some younger ones. It is difficult to judge its precise star formation rate based only on the image.
