The galaxy presents as a largely homogenous spheroid, exhibiting a smooth, relatively featureless morphology. The core region shows a concentrated, bright luminosity, indicative of a potentially dense stellar population or active galactic nucleus. There is a slight ellipticity to the overall shape, suggesting a rotating system. The lack of prominent spiral arms or distinct dust lanes implies that this galaxy may be an elliptical type. The object displays a color gradient from a yellow-white core to more reddish outer regions, potentially representing an older stellar population in the outer regions. The galaxy doesn't appear to be undergoing any major merging events or strong tidal interactions within this observational window. The overall structure suggests a galaxy at a moderately advanced stage of evolution.
