The galaxy presents as a slightly elongated, elliptical or lenticular structure. The central bulge appears smooth and concentrated, exhibiting a yellowish-white hue, possibly indicating an older stellar population. Moving outward from the center, the disk gradually fades into a bluish halo, suggesting the presence of younger, bluer stars within the galaxy's extended regions. There is minimal evidence of distinct spiral arms or significant star formation regions within the disk based on visual inspection alone. It appears to be a relatively isolated galaxy, with no obvious signs of tidal interactions or major mergers impacting its overall morphology. The galaxy demonstrates a fairly smooth overall structure. There may be some minor disturbance in the light distribution, but its presence is questionable.
