The galaxy presents as a fairly smooth structure, with a notable central bulge that appears bright and concentrated. Surrounding this bulge is a disk-like component, though the spiral arms, if present, are not well-defined in this image. The disk exhibits a bluer hue, suggestive of ongoing star formation, particularly when compared to the more yellow/red central bulge. The overall shape is somewhat elliptical but more so an oval shape. There are no obvious signs of major disturbances or tidal features that would suggest a recent major merger event, though there are subtle asymmetries in the outer regions, possibly indicating minor interactions or internal disturbances. The galaxy appears relatively isolated in this field.
