The galaxy presents as a relatively smooth, elliptical morphology with a highly concentrated central bulge.  The light profile appears very uniform, indicating a lack of significant spiral arm structure or distinct star-forming regions. The color is predominantly yellowish-orange, suggesting a stellar population that is evolved, with older, redder stars dominating the light output. There is no obvious indication of active galactic nuclei activity or significant dust lanes. There may be some minor gravitational disturbance as a result of a past merger, but it would be in the very early stages. The galaxy has a high spheroidal component. The object's color suggests low ongoing star formation.
