The galaxy appears to be a spiral type, viewed at a relatively face-on angle. Two primary spiral arms are distinctly visible, exhibiting a moderate winding pattern. There is a hint of additional spiral arms extending from the central region. The arms display a mottled texture, suggesting ongoing star formation. The central bulge is moderately prominent, with a concentrated brightness, though no obvious bar structure is readily apparent in this image. There is a slight suggestion of distortion in the outer regions of the galaxy, possibly indicating a past minor interaction or merger event, although it may also be caused by the resolution of the image. Overall, it shows features common to late-type spiral galaxies.
