The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. The isophotes are elongated with a position angle oriented approximately northwest to southeast. The central region displays a yellowish hue, which may indicate a population of older stars. Moving outwards from the center, the galaxy shows a slight color gradient, becoming somewhat redder in the outer regions, consistent with fainter, cooler stellar populations. There is no discernible spiral arm structure or dust lanes. The galaxy's overall morphology appears undisturbed, lacking any signs of ongoing major merger activity.
