The galaxy presents as a moderately bright, relatively compact object with a largely smooth, elliptical morphology. There appears to be a centrally concentrated bulge exhibiting a yellowish hue, suggestive of an older stellar population. The overall color gradient indicates a possible decline in star formation activity from the center outwards, with bluer colors sparsely present in the outer regions. No prominent spiral arms or distinct morphological features are evident, nor is there any significant evidence of tidal disturbances or ongoing major mergers. The shape appears mostly spherical.