The galaxy presents a generally smooth morphology, appearing elongated in shape, which may indicate it is either an elliptical or a lenticular type. It appears to be in a binary system with another smaller galaxy. The primary galaxy exhibits a bright, concentrated central bulge with a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy display a fainter, bluer tinge, suggestive of some ongoing, albeit possibly subdued, star formation. There is a potential slight disturbance or asymmetry in the galaxy's structure, possibly indicating a past or ongoing interaction with another galaxy, such as the one it seems to be next to. The secondary galaxy appears much smaller, and its faint bluish color indicates the presence of young stars.
