The galaxy presents a generally smooth morphology, exhibiting a central, concentrated region of high luminosity that fades gradually into the surrounding space. The overall shape is elliptical, deviating only slightly from a perfectly circular form. There is minimal visual evidence of spiral arms or distinct disk features; the light distribution appears largely homogeneous. Subtle color gradients are present, with a slightly bluer hue in the central regions, suggesting the presence of younger stellar populations compared to the outer edges, which trend towards redder colors. No strong indications of ongoing major mergers or significant tidal disturbances are observed, though minor asymmetries in the outer isophotes might suggest past interactions or internal dynamical processes.
