The galaxy appears to be a relatively smooth, disk-shaped system seen at a high inclination. The central bulge exhibits a reddish hue, suggestive of an older stellar population. The disk is bluer, indicating younger stars and ongoing star formation, though star forming regions are not strongly pronounced. The galaxy's overall morphology indicates it is likely an early-type spiral or a lenticular galaxy due to the smooth light distribution, although some faint features can be made out. The shape is not perfectly circular, exhibiting a slight elongation. There is no obvious evidence of major interactions or mergers, but the edges of the disk are slightly disturbed.
