The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. Its light profile appears to be largely featureless, lacking prominent spiral arms or distinct dust lanes. There is a color gradient, with the core exhibiting a yellowish hue that fades into a more reddish-brown halo. The galaxy's shape is largely circular, with a small deviation from perfect roundness. There is no evidence of ongoing major mergers or significant tidal disturbances. Based on its color and morphology, this galaxy is likely composed of an older stellar population.
