The galaxy appears to be a spheroidal system. It exhibits a smooth, elliptical morphology with no discernible spiral arm structure or dust lanes. The light profile suggests a concentrated central bulge, with a gradual decline in brightness towards the outer regions. The color is predominantly yellow/gold, indicating a population of older stars and a relatively low rate of ongoing star formation. There is no visual evidence of recent or ongoing merger activity. The galaxy presents a regular and undisturbed appearance.
