The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a concentrated, bright luminosity, suggesting a dense stellar population. The isophotes appear largely regular and concentric, exhibiting a gradual decline in surface brightness moving outwards from the center. There's minimal visible dust or spiral arm features, supporting its classification as a smooth galaxy. Overall, the galaxy appears generally undisturbed with no major signs of an ongoing merger, although some minor irregularity in the outer halo cannot be ruled out. The reddish-yellow color indicates a population dominated by older stars. The overall size appears moderate.
