The galaxy appears to be an elliptical type, exhibiting a smooth, somewhat elongated morphology. Its light profile suggests a centrally concentrated spheroid with a gradual decrease in brightness towards the outer regions. The galaxy appears to be yellow/orangeish in color, suggesting an older stellar population. There is no evidence of spiral arms or prominent dust lanes, and the overall structure seems undisturbed, with no obvious signs of any major merger events or strong tidal interactions. There may be some signs of minor disturbances, or a faint disk component, but the morphology is primarily spheroidal.
