The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated luminosity, appearing almost spheroidal. The radial color gradient suggests a transition from a yellower, older stellar population in the core to slightly bluer hues in the outer regions of the galaxy. While some very subtle irregularities in the outer regions might suggest minor tidal interactions, the overall structure appears undisturbed, with no prominent spiral arms or bar-like features visible. There is no obvious indication of active galactic nucleus activity based solely on the image, though higher resolution data would be needed to definitively rule this out. The moderate redshift implies a substantial distance. The estimated size is a few kiloparsecs. The overall impression is that of a relatively massive galaxy, possibly in the early stages of its formation.
