The galaxy presents as a concentrated, ellipsoidal object. A bright, relatively smooth central region dominates the morphology, with a gradual decrease in luminosity extending outwards. The color profile suggests a bluer core transitioning to redder hues in the outer regions. There appears to be a slight asymmetrical distribution of light, but no distinct spiral arm structures or prominent dust lanes are visible. There is marginal evidence of possible tidal disturbances or interactions occurring with a low chance that the disturbance is a merger. The galaxy's overall appearance points towards it being an elliptical or lenticular galaxy type.
