The galaxy presents as a relatively smooth, elliptical morphology. There is a concentration of light towards the center of the galaxy, suggesting a prominent galactic nucleus. The light gradually diffuses outward, with no distinct spiral arm structures visible. The galaxy exhibits a color gradient; the core appears more yellow, transitioning to redder hues in the outer regions. This implies the central bulge is dominated by older stellar populations, while the outskirts may contain a mix of stellar ages, or dust reddening. Overall, the galaxy is roughly circular, with only slight deviations from perfect symmetry. There is no evidence of any major ongoing merging events or significant tidal disturbances, although there might be some minor disturbances.