The galaxy exhibits a generally elliptical morphology, though significant disturbances are visually apparent. The central region presents a high degree of luminosity with a yellowish hue, suggesting a concentration of older stellar populations. Extending outward from this central bulge is a fainter, more diffuse halo. A discernible disk-like structure is observed, but it appears distorted, possibly due to interactions with other galaxies or internal dynamic processes. Evidence of merging activity is prominent. There are irregularities in the galaxy's shape, including tidal tails or bridges of stars and gas extending from the main body. The disturbances suggest the presence of ongoing or recent star formation. The blue color of the outer regions indicates the presence of younger, hotter stars. Dust lanes may also be present, obscuring some of the light from background stars. The system has an estimated diameter of about 12,000 lightyears. The galaxy appears to have a mass of approximately 50 billion suns.
