The galaxy appears as a relatively small, elongated structure. Its morphology suggests an elliptical or lenticular classification, exhibiting a smooth, diffused light distribution without prominent spiral arms. There is a slight color gradient across the galaxy, hinting at variations in stellar populations or dust content, though this is subtle. The galaxy's profile is moderately elongated with its major axis being a few times larger than its minor axis. There does not appear to be any evidence of an active galactic nucleus or recent major merger activity based on the current image resolution.
