The galaxy appears to be an elliptical galaxy. It exhibits a generally smooth morphology with a high degree of central concentration. It has a spheroidal shape, appearing mostly round, with a slight yellow-orange hue indicative of an older stellar population. There is little evidence of spiral arms or significant dust lanes, suggesting a quiescent or post-starburst system with a relatively low rate of ongoing star formation. There is no sign of an active galactic nucleus or evidence of major merger activity. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or nearby companion galaxies in the immediate vicinity.
