The galaxy presents as a single, concentrated light source, with a smoothly decreasing luminosity profile extending outwards from a bright, well-defined core. The object exhibits a nearly circular morphology, with no obvious spiral arm structures or bar features visible. The color of the galaxy appears generally yellowish, with a hint of red in the outer regions and a brighter white-yellow core, which may suggest the presence of an older stellar population and a possible lack of significant ongoing star formation. There is no strong evidence for significant dust lanes or recent merger activity. Given the smooth appearance and color, a classification of elliptical galaxy, or potentially a lenticular galaxy seen face-on, may be appropriate. The galaxy is relatively compact. There appears to be no obvious sign of a central active galactic nucleus.
