The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is somewhat elliptical, tending toward a more rounded shape but deviating slightly. There is no strong indication of spiral arm structure or a prominent disk from the visual data. The galaxy appears largely undisturbed, exhibiting no obvious signs of a major merger or significant tidal disruption. Subtle asymmetries or minor irregularities might be present in the galaxy's outer regions. The color gradient indicates a population dominated by older stars. Star formation is not expected to be high, although some is possible.
