The galaxy presents as a relatively smooth, elliptical structure. There is little indication of spiral arms or significant dust lanes. The central region exhibits a high degree of luminosity, appearing as a bright, concentrated core. The overall shape is predominantly round, with only a slight deviation towards a more elongated form. There is no obvious evidence of recent or ongoing major mergers or significant tidal disturbances, though a minor disturbance or interaction cannot be ruled out given the image resolution. The galaxy's color appears to be relatively uniform, with a subtle shift towards redder hues, which could indicate an older stellar population and a relatively low rate of current star formation.
