The galaxy presents as a centrally concentrated, elliptical system. Its overall color profile indicates a relatively older stellar population. The central bulge appears bright and smooth, suggesting a high density of stars. There's a slight hint of a diffuse halo surrounding the central region. The galaxy has a subtle blueish color to it, indicating low-level star formation. There is no clear spiral arm structure or evidence of significant dust lanes visible. The galaxy's morphology suggests it is a relatively isolated system that is not currently undergoing any major merging events.
