The galaxy appears to be a relatively compact object with a noticeable central bulge. The light distribution is dominated by a smooth, centrally concentrated component, suggesting an elliptical or lenticular morphology. There is some indication of a faint, extended disk surrounding the central region. The disk appears slightly tilted with respect to our line of sight. The color gradients suggest a change in stellar population, with a bluer core transitioning to redder outer regions. There is some evidence of a minor disturbance or tidal feature in the disk, though it is not a strong or obvious interaction. The overall shape seems roughly round to slightly elongated.
