The galaxy presents a generally smooth morphology, with a slightly elongated, elliptical shape. The core exhibits a bright, concentrated luminosity, transitioning to a dimmer, more diffuse halo. Coloration suggests a population of older stars, leaning towards redder hues. No distinct spiral arm structures or prominent dust lanes are discernible. There is a slight asymmetry in the outer regions of the galaxy, but no immediate signs of major ongoing merging events or tidal disturbances are clearly observed.
