The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile with a bright, diffuse core, suggesting a dense stellar population. The galaxy appears mostly featureless in the available image, lacking prominent spiral arms or significant dust lanes. The color gradient indicates a population of older stars, contributing to its yellowish-red hue. There's no obvious evidence of active galactic nuclei activity or recent star formation. The overall morphology suggests a galaxy that has undergone significant stellar evolution and is approaching a quiescent state. Its round shape indicates it is not viewed edge on, and there are no merging events impacting the galaxy.
