The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the galaxy's structure, exhibiting a yellowish-white hue, likely indicating an older stellar population. Surrounding the bulge, a less concentrated disk is present, displaying a bluer coloration. This may be the presence of younger, hotter stars within this region. A faint reddish patch is seen on the upper-left section of the disk, possibly indicating a region of active star formation or dust obscuration. The overall shape is somewhat round, though there is slight asymmetry in the outer regions, suggesting a minor gravitational interaction or disturbance. There is no clear evidence of a major ongoing merger, although subtle irregularities hint at past interactions.
