The galaxy presents a predominantly smooth morphology, exhibiting characteristics consistent with an elliptical or lenticular type. The light profile displays a centrally concentrated bulge that dominates the overall luminosity. There is some apparent elongation along a discernible axis, suggesting a departure from perfect sphericity. Subtle color gradients are observable, with a yellowish hue in the central regions, possibly indicative of an older stellar population. Fainter, bluer regions are observed in the surrounding halo. No prominent spiral arms or distinct dust lanes are apparent. The overall structure appears relatively undisturbed, with no major signs of ongoing merger activity or significant tidal distortions.
