The galaxy presents as a slightly elongated, diffuse object with a central concentration. The overall color is a yellowish-orange, possibly indicating an older stellar population with lower rates of ongoing star formation. There appears to be a subtle asymmetry in the distribution of light, potentially suggesting minor gravitational interactions or internal disturbances. The galaxy exhibits a smooth appearance, with a large fraction of the object being concentrated around the central bulge. There is no clear evidence of spiral arms or a well-defined disk structure. The overall morphology suggests a system that is moderately massive with moderate star formation.
