The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. A bright, unresolved core dominates the emission, surrounded by a more diffuse halo. The light profile appears relatively symmetrical. There is very little visual evidence of spiral arm structures or significant dust lanes. The color gradient suggests a population of older stars, with the central region appearing more yellowish-orange compared to the outer regions. The overall appearance suggests a galaxy that has largely completed its star formation, consistent with a passively evolving system. Subtle asymmetries in the outer regions cannot be ruled out but are not prominent. The galaxy is well-defined, suggesting it's not undergoing any major mergers.
