The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually diminishes in intensity towards the outer regions. The overall shape appears somewhat elongated, suggesting a possible oblate spheroid morphology, with the major axis oriented horizontally within the frame. There is no clear evidence of spiral arms or significant dust lanes, though the image resolution limits definitive statements. The color suggests a population dominated by older stars, implying a low rate of ongoing star formation. No signs of significant tidal disturbances or ongoing merger activity are immediately apparent.
