The galaxy presents as a roughly elliptical, relatively smooth object, exhibiting a concentrated central bulge that gradually fades into a more diffuse halo. The color profile is dominated by yellowish-white hues in the center, suggesting an older stellar population. There's a subtle shift toward redder tones in the outer regions, which might indicate ongoing or recent star formation with associated dust obscuration. No distinct spiral arm structures or significant morphological irregularities are readily apparent. The galaxy appears isolated, showing no immediate signs of tidal distortion or interaction with other galaxies.
