The galaxy exhibits a prominent disk structure with well-defined spiral arms. These arms appear somewhat flocculent, displaying varying degrees of tightness in their winding. Two main spiral arms emanate from the central region, with indications of further branching and substructure. The central bulge is moderately sized and presents a yellowish hue, suggesting an older stellar population. Dust lanes are discernible within the spiral arms, particularly on the near side, obscuring some of the starlight. The disk appears slightly inclined to our line of sight, allowing for a partial view of the spiral structure. The overall color of the disk is bluish, indicative of ongoing star formation. No signs of a major merger event are immediately apparent, although some minor tidal disturbances cannot be ruled out. The galaxy has an overall elliptical shape. A strong central bar bisects the galaxy.