The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The shape is approximately elliptical, appearing mostly rounded with a slight deviation toward an in-between shape. There is little evidence of spiral arm structure or significant disk features. The light distribution suggests a primarily spheroidal component. The galaxy exhibits a yellow-white hue, potentially indicating a stellar population dominated by older stars and a reduced rate of ongoing star formation. There is no obvious dust lane. The galaxy does not show clear signs of tidal disturbances or interaction with other galaxies. The overall appearance suggests this is a fairly evolved galaxy.
