The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its light profile suggests an old stellar population, with a predominantly yellowish-orange hue, indicative of evolved stars. There is no clear evidence of spiral arms, a bar, or significant dust lanes. The galaxy presents a highly rounded shape. Possible minor disturbances are very subtle, without any obvious signs of major tidal interactions, mergers, or significant star formation. The galaxy possesses a substantial stellar mass. The colors suggest it is relatively quiescent, with low star formation rate.
