The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated luminosity profile, with a smooth, diffuse halo. The core region demonstrates a high degree of spheroidal symmetry. The light distribution appears to be relatively uniform, with no prominent spiral arm structures or distinct dust lanes immediately apparent. There is evidence of a slight elongation along a particular axis. Color gradients suggest a redder central region, potentially indicative of an older stellar population within the bulge. Fainter, bluer light is visible in the outer regions, possibly arising from recent star formation. There is no indication of significant tidal disturbances or ongoing mergers. Overall, the galaxy appears to be a relatively evolved system.
