The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The central region appears to be dominated by an intense concentration of light, suggesting a significant stellar density and likely an older stellar population. Proceeding outward, the light intensity gradually diminishes with a nearly complete lack of apparent substructure such as spiral arms or distinct dust lanes. The ellipticity of the galaxy is moderate, with the ratio of the major to minor axis being approximately 3:1. There's a subtle color gradient, shifting from a yellow core to a redder outer region, suggesting a radial variation in stellar population and/or dust content. There is no evidence of any current or recent major merger activity.
