The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge. There is no apparent spiral arm structure or a well-defined disk. The light distribution suggests a moderate degree of roundness, rather than a highly elongated or cigar-shaped form. No significant tidal distortions or nearby interacting companions are visibly apparent. Overall, the galaxy's morphology indicates that it has likely undergone past mergers. Its light appears to be largely generated from older stellar populations. A small amount of new star formation may be present. This galaxy is likely a somewhat massive system.
