The galaxy presents as a largely featureless elliptical system. It exhibits a centrally concentrated light distribution with a smooth, gradual decline in luminosity towards the outer regions. The core appears bright and unresolved, indicative of a dense stellar population or possible active galactic nucleus. There is a slight elongation to the overall shape but it is mostly round. There is minimal evidence of spiral arms or distinct disk structures. The colour appears to be a somewhat uniform distribution of light blue/white light. The galaxy displays no signs of major disturbances or ongoing mergers; however, there are faint indications of minor asymmetries or tidal features that may warrant further investigation. The galaxy appears relatively isolated based on the surrounding field.
