The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an elliptical or lenticular morphology, lacking any distinct spiral arm structures or a prominent disk. The light distribution is generally even, with a gradual fading towards the edges. The core region displays a brighter, more intensely blue hue, which may suggest a concentration of younger, hotter stars or a central active galactic nucleus. There appears to be a subtle, somewhat asymmetric extension in the galaxy's outer regions, possibly indicating a minor interaction or tidal disturbance, though no major mergers or significant distortions are readily apparent. Overall, the galaxy appears to be relatively undisturbed and evolved, exhibiting characteristics consistent with a population of older stars.
