The galaxy presents as a system with a notable concentration of light towards the center, suggesting a significant central bulge. The galaxy exhibits an overall ellipsoidal shape, with a relatively smooth appearance. There is some evidence of asymmetry, with a slightly elongated structure, which may indicate tidal interactions or internal disturbances. The color distribution is primarily yellow-orange across the galaxy, which could indicate an older stellar population and relatively low ongoing star formation. There is potential for this galaxy to be a galaxy in the process of merging with another, smaller galaxy.
