The galaxy presents an overall elliptical morphology, with a somewhat elongated shape. It displays a smooth appearance with little evidence of distinct spiral arms or significant dust lanes. The galaxy’s central region appears slightly brighter, suggesting a concentration of stars and possibly a central bulge. There is a hint of a disk-like structure surrounding it. The color appears to be primarily composed of light toward the redder end of the spectrum, which may indicate an older stellar population with suppressed star formation activity. There is a potential interacting galaxy or tidal disturbance event taking place, which is hard to distinguish. There is also some possible minor disturbance evident in its morphology. It's a relatively compact galaxy, not exhibiting a large, diffuse halo.
