The galaxy presents a somewhat smooth, round appearance. The central region exhibits a concentration of yellow light, suggesting an older stellar population or the presence of dust obscuration. Moving outwards from the core, a faint, diffuse halo is visible. There are also several more diffuse areas of light, perhaps a feature of a disk. The galaxy does not show clear spiral arm structure or a distinct bar. There are some irregularities in the distribution of light, suggestive of minor disturbances or ongoing interactions. Overall, the galaxy appears to be a relatively massive system.
