The galaxy presents as a spheroid-shaped object with a smooth, featureless morphology. The color appears to be predominantly yellowish-orange, suggesting an older stellar population with a relatively low rate of current star formation. There is evidence of a possible minor interaction or merger event, indicated by a slight asymmetry or distortion in the overall shape and the presence of a fainter, smaller component in close proximity to the main galaxy body. The size of the galaxy is relatively compact.
