The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. It appears to be primarily spheroidal in shape, exhibiting a high degree of roundness in its overall structure. There's no readily apparent spiral arm structure or distinct disk component. The light appears more reddish, possibly indicating a population dominated by older stars. No major mergers or tidal disturbances are visibly distorting its form. The galaxy appears relatively isolated, with no obvious close companions or interacting systems.
