This galaxy appears to be a lenticular or early-type spiral, exhibiting a smooth, disk-like morphology without prominent spiral arms. The light is concentrated centrally, with a gradual decrease in brightness towards the outer edges. There is a faint, elongated structure, indicating a disk seen at an oblique angle. The color gradient suggests an older stellar population. The galaxy shows a relatively homogenous color profile, possibly indicative of ongoing, but subdued, star formation. The dust lanes are not prominently visible.
