The galaxy presents as a somewhat smooth, elliptical-like system with an apparent redshift. It displays a concentrated central bulge that transitions gradually outward into a less defined, diffuse halo. The galaxy exhibits an overall elongated morphology, with the major axis oriented at an angle to the image frame. There is a subtle color gradient, with the central region appearing more yellow/white, suggesting an older stellar population, while the outer regions show a slight blue tint, potentially indicating younger stars. The absence of well-defined spiral arms or dust lanes is noticeable. Some minor disturbances can be observed, and the galaxy has a substantial mass.
