The galaxy presents as a disk-shaped structure, elongated with an axis ratio of approximately 0.46. Its major axis is oriented at roughly 62 degrees relative to the image frame. The central bulge appears substantial and exhibits a smooth profile. The galaxy shows a clear color gradient, transitioning from bluer hues in the outer disk to redder tones towards the central bulge. This color variation suggests a difference in stellar populations, with younger, bluer stars potentially dominating the disk and older, redder stars concentrated in the bulge. Star formation appears present, but at a low intensity. The overall smooth appearance and the axis ratio suggest that this galaxy is a late type spiral with flocculent arms or a lenticular galaxy. There are no signs of any major merger, nor any significant tidal disturbances in its overall structure.
