The galaxy presents an overall elliptical morphology, though a slight asymmetry is apparent, possibly indicative of an interaction or recent merger. The central region exhibits a bright, concentrated core suggestive of an older stellar population, implied by its yellower color. Moving outward, the galactic disk appears relatively smooth with a subtle gradation in color and intensity. The outer regions transition towards a fainter, bluer hue, hinting at ongoing star formation in these areas. There may be some minor disturbances to the disk from a possible ongoing merger, which would account for its disturbed morphology. There is an extended halo, but it is hard to make any deductions.
