The galaxy presents an elliptical morphology, appearing generally smooth in structure. The central bulge exhibits a concentrated brightness, indicative of a high stellar density. There is a slight elongation along one axis, but the overall shape is more rounded than cigar-shaped. The galaxy has a yellow/red hue, suggesting an older stellar population and relatively low ongoing star formation. Possible minor disturbances or interactions may be present, but the dominant impression is of a relaxed, undisturbed system. No distinct spiral arms or prominent dust lanes are discernible.
