The galaxy presents as a somewhat elliptical, relatively compact structure. There is a discernible central bulge that appears yellowish-white, suggesting a population of older stars. Surrounding the bulge, a faint, diffuse disk is observed, exhibiting hints of bluer colors, possibly indicating more recent star formation, albeit at a low rate. The disk appears slightly disturbed, with a subtle asymmetry visible. There is no strong evidence of a grand design spiral structure, although there may be faint, poorly defined arms. The galaxy does not appear to be undergoing a major merger, but there may be a minor interaction or disturbance affecting its overall morphology.
