The galaxy appears as a centrally concentrated object with a relatively smooth morphology. The galaxy exhibits a slight elongation. There is an apparent colour gradient, the central region is a green hue which transitions towards the outer edges that appear bluish in colour. The overall colour suggests recent or ongoing star formation, albeit at a moderate rate, based on its overall luminosity. There's no readily discernible spiral structure or bar. No significant tidal disturbances or signs of a major ongoing merger are apparent. The galaxy's structure is not perfectly symmetrical, and there might be some subtle disturbances indicating either a minor interaction or internal dynamics influencing its shape. The lack of strong features suggests that the galaxy is likely an elliptical or lenticular type with a relatively evolved stellar population in the central region.