The galaxy presents as a relatively smooth, elliptical-like object. The central region exhibits a concentrated luminosity with a yellowish-white hue, suggesting an older stellar population. There is a subtle color gradient moving outward from the core, with the outer regions showing hints of redder tones, which may indicate the presence of dust or a slightly different stellar population mix. No prominent spiral arms or distinct features are discernible; the overall structure appears largely amorphous. There is very little blue, indicating low star formation rate. The overall round appearance and lack of significant disturbances suggest a relatively relaxed morphological state.
