The galaxy appears to be a fairly smooth, elliptical structure with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting an older stellar population with relatively low levels of ongoing star formation. The galaxy is generally round, displaying no obvious signs of spiral arms or significant morphological disturbances. There are no apparent signs of a major merger event or tidal features. The galaxy's overall smooth morphology suggests that it has likely reached a stage of relative quiescence in its evolution.
