The galaxy presents as a slightly elongated, diffuse object. It exhibits a distinct reddish hue overall, suggesting a stellar population dominated by older, redder stars or significant dust obscuration. There is minimal evidence of spiral arm structure or a well-defined nucleus. The light distribution appears relatively smooth and concentrated, although faint irregularities are present, hinting at minor disturbances within the galaxy, or the possibility of an interaction with a companion galaxy. The color distribution is fairly uniform, with no strong evidence of recent star formation regions dominating the galaxy. Overall, the galaxy appears to be an elliptical galaxy or a quiescent spiral galaxy viewed at a high inclination angle. Further spectroscopic data would be required to confirm its classification and determine its redshift, star formation rate, and chemical composition.
