The galaxy presents a generally smooth, elliptical morphology, with a bright, concentrated central bulge. There is a notable color gradient, with the central region exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions appear slightly bluer, hinting at the presence of some younger, hotter stars, though the overall star formation rate appears relatively low. The galaxy's shape is more in between, with a slight elongation, but is not distinctly cigar-shaped or round. There are no obvious signs of major disturbances or ongoing merging events, with only slight asymmetry visible in the outer regions.
