The galaxy presents as an elliptical morphology. It appears largely featureless, with a smooth, diffused light distribution. The galaxy exhibits a notably round shape. The color profile suggests a dominant population of older stars, with a yellow-red hue indicative of minimal ongoing star formation. There are no obvious signs of spiral arm structures, dust lanes, or tidal disturbances to suggest recent merger activity or significant ongoing interactions. Overall, this galaxy seems to be a relatively quiescent system with a well-defined, centrally concentrated structure.
