The galaxy presents as a yellowish-orange elliptical-like structure. It exhibits a centrally concentrated bright core which gradually fades towards the outer regions. There appears to be a slight extension of the galaxy along one axis, giving it a somewhat elongated, rather than perfectly spherical, shape. There are no apparent spiral arms or well-defined dust lanes visible in this image. The overall morphology is relatively smooth with minimal signs of significant disturbances or mergers. The color suggests a stellar population dominated by older, redder stars and a relatively low rate of ongoing star formation. The estimated size indicates a substantial but not exceptionally large galaxy.
