The galaxy presents an overall elliptical morphology, though it appears somewhat elongated. Its central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. Proceeding outwards, a diffuse halo emanates from the core. The color profile indicates a mix of stellar populations, with the core showing a slightly redder hue that could signify older stars or dust obscuration, while the outer regions display bluer tones, possibly due to the presence of younger, hotter stars. Some minor structural features are also visible, but are too unclear to assess accurately the ongoing evolutionary processes. The galaxy is quite massive and its star formation rate is relatively moderate.
