The galaxy presents a generally smooth, elliptical morphology with an apparent bulge-like central region. Its color profile shifts from a yellowish-orange at its core to a slightly bluer hue in the outer regions. This color variation may suggest differing stellar populations or dust distribution within the galaxy. I observe faint, diffuse extensions emanating from the central body, potentially indicating tidal disturbances or ongoing interactions with other galaxies. The general shape appears to be more oval than circular. The light distribution appears relatively even, except for the brighter central region. There is also evidence of merging features.
