The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge exhibiting a yellowish hue. Two faint, extended features appear to emanate from either side of the central region, suggesting possible tidal tails or disturbed spiral arms. These features display a slight reddish tint, potentially indicating older stellar populations. The overall shape is somewhat elongated. The galaxy exhibits minimal evidence of ongoing, intense star formation, instead appearing to be comprised primarily of older stellar populations. The system shows potential signs of minor gravitational disturbance.
