The galaxy presents as a concentrated, largely featureless object. It exhibits a smooth, elliptical morphology, with a centrally condensed bulge dominating the light profile. The core is a bright yellow, potentially indicating an older stellar population, likely a result of minimal current star formation. There may be some faint evidence of extended structure or a very diffuse disk. There is some subtle colour variation that can be seen in the disk that may suggest slight dust extinction. No tidal features or signs of recent major mergers are readily apparent, indicating it is likely an undisturbed system.
