The galaxy presents as a centrally concentrated, smooth object. Its morphology appears elliptical, exhibiting a somewhat flattened spheroidal shape, though it could also be a spiral viewed face-on. The light distribution transitions gradually from a bright core to a fainter, extended halo, with no obvious substructure suggestive of spiral arms or a bar. The color is predominantly blue-white in the central region, hinting at the presence of younger stars. The outer regions seem to trend towards redder hues, indicating the likelihood of an older stellar population. There are no indications of significant tidal features, major disturbances or ongoing major mergers, although I do note what appears to be a minor asymmetrical disturbance extending in the upper left part of the galaxy. Overall, it has a smooth, mostly homogenous structure, with no strong evidence of star formation or major active galactic nuclei activity.
