The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The galaxy has a notable deviation from circularity, with its shape appearing somewhat elongated. There is no obvious spiral arm structure or significant dust lane features visible. The color gradient suggests a relatively uniform stellar population, potentially dominated by older, redder stars. The core region shows a high surface brightness, indicating a possible active galactic nucleus or a dense concentration of stars. Faint diffuse light extends outwards from the central region, with a fairly sharp cutoff at the edges, indicating a well defined galaxy edge. Overall, the galaxy appears to be a relatively massive early-type galaxy at a moderate redshift.
