The galaxy presents as a single, concentrated luminous structure. Its morphology is predominantly smooth, with a notable absence of distinct spiral arms or a well-defined disk. The light distribution suggests a spheroidal shape, appearing largely rounded. The central region exhibits a high surface brightness, indicative of a dense concentration of stars, and is emitting yellow light. There is no apparent dust lane obscuring the view of this galaxy. The surrounding areas of the galaxy gradually diminish in luminosity, with no clear signs of ongoing major star formation, major disturbances, or a recent merger.
