The galaxy appears as a centrally concentrated, smooth object with a generally elliptical morphology. It presents a yellowish-orange hue, suggesting a dominant population of older stars and a relative paucity of ongoing star formation. The light distribution is fairly uniform, lacking any prominent spiral arm structures or distinct features. The galaxy does not appear to be strongly interacting or undergoing a major merger, although there might be a minor asymmetry that bears additional inspection. The observed color indices imply a moderate redshift. The estimated physical size corresponds to a relatively large galaxy.
