The galaxy presents as a smooth, elliptical structure. Its morphology appears to be elongated, exhibiting a cigar-like shape. The central region displays a bright, concentrated luminosity, suggestive of a prominent galactic bulge. The colour profile indicates a dominance of older stellar populations, with a yellowish-orange hue. There is no visible spiral arm structure or significant dust lane obscuration. There appears to be a smooth brightness gradient from the core to the outer edges. Close inspection does not suggest any major signs of ongoing merger activity or significant tidal disturbance, though subtle asymmetries in the outer regions cannot be entirely ruled out. Overall, the galaxy appears to be relatively isolated and quiescent.
