This galaxy presents as a relatively smooth, elliptical structure. A concentrated bulge is visible, exhibiting a warmer, yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer tint, potentially indicating the presence of younger stars or ongoing star formation, although this activity appears subdued. The overall shape leans towards a somewhat elongated, "in-between" spheroidal form rather than a perfectly circular or distinctly cigar-shaped morphology. There is no immediately obvious evidence of major mergers or significant tidal disturbances affecting its structure.
