The galaxy presents a moderately elliptical morphology, appearing neither perfectly spherical nor highly elongated. A central bulge region is visible, exhibiting a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy display a bluer color, potentially indicative of ongoing star formation. There are some slight irregular features and disturbances present, suggesting possible interactions or mergers in the galaxy's past. Overall, the galaxy appears to be relatively smooth in structure, with no prominent spiral arms or other distinct features readily observable.
