This galaxy exhibits a largely smooth morphology, with no readily apparent spiral arm structures or significant dust lanes visible. The galaxy appears approximately round, displaying a high degree of circular symmetry. There is a slight elongation that might suggest a transition towards a more elliptical shape, however, the galaxy is mostly spherical in overall form.

The color of the galaxy leans towards the bluer end of the spectrum. This implies a younger stellar population. The evenness of color suggests that star formation is occurring uniformly throughout the galaxy, or that the stars are uniformly distributed within the galaxy's radius.

Based on visual inspection, there is no obvious evidence of ongoing major merger activity or significant tidal disturbances. The light distribution appears fairly centralized, with no distinct core or noticeable irregularities. The galaxy seems undisturbed and relatively isolated in its evolution.
