The galaxy presents a generally elliptical morphology, appearing somewhat flattened with a major axis extending approximately horizontally in the frame. The light distribution suggests a smooth profile without distinct spiral arm structures. The central bulge exhibits a high surface brightness, gradually decreasing towards the outer regions. The galaxy's color appears relatively uniform across its structure, indicating a stellar population with a moderate range of ages. There might be subtle color variations, with the central region appearing slightly yellower compared to the outer regions, possibly indicating a higher concentration of older stars in the core. There's no strong evidence of significant dust lanes or active star formation regions discernible in the image. The overall appearance is consistent with an early-type galaxy at a moderate distance, showing no obvious signs of recent mergers or significant interactions.
