The galaxy presents as a relatively smooth, elliptical object with a dominant central bulge. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. There is little evidence of spiral arm structures or significant dust lanes, indicating a lack of recent major mergers. The color index suggests a population of older stars. The galaxy shows a largely featureless morphology, with no clear signs of active star formation regions. The apparent shape is nearly circular, supporting the classification as an elliptical galaxy.
