The galaxy presents as a relatively smooth, elongated structure, strongly suggesting an elliptical morphology. The light distribution is centrally concentrated with a noticeable bulge. Color gradients are present; the central region exhibits a yellowish hue, possibly indicative of an older stellar population, while the outer regions appear bluer, suggesting the presence of younger stars, or perhaps a weak disk component. There is a slight asymmetry to the outer regions, but the overall shape is largely undisturbed, with little indication of major mergers or tidal interactions. The galaxy is moderately bright, with an apparent magnitude suggesting a substantial luminosity at its inferred redshift.
