The galaxy appears as a relatively smooth, centrally concentrated object with a round morphology. The color profile suggests a dominant population of older stars, with a yellowish hue. There is little evidence of spiral arm structure or significant dust lanes. The overall light distribution is fairly symmetric, indicating a lack of major ongoing merger activity. The galaxy appears to be a well-formed, spheroidal system, possibly an elliptical galaxy or a lenticular galaxy seen face-on. It exhibits a gradual decrease in surface brightness from the core to the outer regions.
