The galaxy exhibits a moderately bright central bulge that appears nearly spherical. There is some evidence of a disk component surrounding the bulge, although it appears somewhat disturbed or irregular. The color gradient suggests a higher concentration of older stellar populations in the central bulge, indicated by its relatively redder hue. The outer regions show bluer colors, suggesting ongoing star formation or the presence of younger stellar populations. The overall morphology appears to be that of a spiral galaxy, with a faint indication of spiral arm structures. The edges of the disk are not well-defined, possibly indicating tidal interactions or distortions due to mergers. Evidence of a possible minor merger event may be visible.
