The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated, bright central bulge characterized by a yellowish hue, suggestive of an older stellar population. A fainter, somewhat elongated halo surrounds the central region, extending primarily along one axis, potentially indicating tidal interactions or a nascent disk structure. There are slight color variations within the halo, with hints of bluer regions interspersed amongst the more neutral tones. These patches could represent regions of recent star formation. Overall, the galaxy appears to be a mature system undergoing relatively quiescent evolution.
