The galaxy presents as a concentrated central structure exhibiting a smooth morphology. The light distribution appears relatively even across the core, suggesting an older stellar population. There appears to be ongoing or recent merger activity with several distinct light concentrations. The main body exhibits a yellowish hue, indicative of evolved stars. Signs of disturbance are noted, including asymmetric light distribution in the outer regions. The overall shape appears generally round, although perturbations suggest tidal interactions. Star formation appears to be suppressed.
