The galaxy presents as a relatively smooth, disk-shaped structure, elongated in appearance and consistent with an edge-on or highly inclined disk galaxy. A bright, concentrated central bulge is evident, exhibiting a yellowish-red hue, possibly indicating an older stellar population and dust obscuration. Fainter blue regions are observed along the outer edges of the disk, suggestive of ongoing star formation within spiral arms. The overall morphology suggests a classification leaning towards an Sa or Sb spiral galaxy, though a clear spiral arm structure is not readily discernible in this image. There is no prominent evidence of major mergers or significant tidal disturbances.
