The galaxy presents a largely smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid with a radial decrease in luminosity. The color profile is relatively uniform across the galaxy, with a slight bluing in the outer regions. There is no clear evidence of spiral arm structure, bars, or a prominent dust lane. The lack of distinct features, along with its smooth appearance, suggests that the galaxy is a relatively undisturbed system, likely an elliptical or S0 type. The overall appearance indicates that the galaxy is likely composed of an older stellar population, with ongoing or recently concluded star formation. There are no indications of a significant merger event.
