The galaxy appears to be a relatively smooth elliptical type, exhibiting a generally elongated, cigar-shaped morphology. It demonstrates a centrally concentrated light distribution, with a core region displaying a brighter, slightly reddish hue. Moving outward from the center, the galaxy's color shifts towards a bluer shade. This may suggest ongoing, though modest, star formation activity in the outer regions compared to the more quiescent central bulge. There is no strong evidence of spiral arm structure or significant tidal disturbances, although a slight asymmetry in the outer isophotes cannot be entirely ruled out. Overall, the galaxy presents as a well-formed and relatively undisturbed system.
