This galaxy appears to be a spiral type, though the inclination obscures a clear view of its structure. A flattened disk is visible, oriented roughly horizontally in the image.

One region of the disk appears brighter and more concentrated, possibly indicating a bulge or a denser region of star formation. This region displays a yellowish hue, suggesting an older stellar population. The rest of the disk appears more diffuse and blueish, which may correspond to more recent and ongoing star formation.

There is some evidence of asymmetry in the disk's shape, with a slight warp or irregularity noticeable on one side. This could be the result of tidal interactions with another galaxy or a past merger event.

The overall color suggests a moderate redshift, indicating it's a moderately distant object. The size appears relatively compact, though a more precise determination would require redshift-independent distance measurements.
