The galaxy presents as a single, mostly homogenous, and largely featureless elliptical object. The core is bright and concentrated, with a radial decrease in luminosity towards its edge. Its shape is generally rounded, with an intermediate color index, exhibiting a subtle shift towards redder hues. There appears to be no significant evidence of spiral arms or a prominent disk structure. There is no clear evidence of a major ongoing merger event or significant tidal disturbance. The galaxy exhibits a level of smoothness, suggesting a relatively evolved stellar population.
