The galaxy presents as a moderately bright elliptical, exhibiting a smooth, largely featureless morphology. The central bulge appears prominent and concentrated, displaying a warmer, yellowish hue which suggests an older stellar population. A fainter, bluer halo surrounds the bulge, indicating the presence of younger, hotter stars, although the proportion of these stars appears relatively low. Overall, the galaxy exhibits a general spheroidal shape, with a mild extension along one axis. There's no immediately obvious evidence of spiral arms or active star formation regions, nor are there any signs of significant ongoing mergers or tidal disturbances.
