The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a bright, concentrated luminosity, suggesting a significant stellar population. Moving outwards from the core, the light gradually diffuses into a fainter halo. There is a suggestion of subtle, elongated shape rather than perfect circular symmetry, hinting at a possible deviation from a purely spherical form. No obvious spiral arm structures or prominent dust lanes are discernible. The color gradient moves from yellow-white near the core to a slightly redder hue in the outer regions. There are very slight irregularities or minor disturbances in its overall structure.
