The galaxy presents as a relatively smooth, elliptical-like structure. The object exhibits a concentrated central bulge that appears yellowish in color, indicating a population of older stars. There is a lack of prominent spiral arm structures or dust lanes that would be associated with ongoing, significant star formation. The smooth light distribution suggests a high degree of symmetry. Faint hints of bluer light emanate from the outer regions of the galaxy, which may suggest sparse pockets of younger stars. The morphology leans toward spheroidal, showing high roundness. There's evidence of some gravitational interaction or recent merger activity due to the slight asymmetry and disturbed outer regions. The overall color profile suggests a red and dead galaxy with little ongoing star formation.
