The galaxy presents a generally elliptical morphology, although some structure is discernible within the disk. Its orientation is oblique relative to the observer's line of sight. A bright, concentrated nucleus is apparent, surrounded by a smooth, extended bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Fainter, bluer spiral arms extend outwards from the central region. These arms show some patchiness, possibly indicating ongoing star formation regions. A hint of a dust lane is visible on the near side of the disk, partially obscuring the light from the bulge. The overall structure is moderately disturbed, but no clear signs of an ongoing major merger are evident.
