The galaxy presents a generally elliptical morphology, appearing rather smooth in overall structure. The core region exhibits a concentrated brightness, suggesting a well-defined central component, possibly a galactic nucleus. A subtle color gradient is observed, transitioning from a yellowish-white core to a bluer, more diffuse outer region. This color variation may indicate differences in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the outer regions. While appearing smooth, there's a hint of a slight disturbance or asymmetry in the outer reaches of the galaxy, which could be indicative of past or ongoing interactions, though no major merging features are obvious. The overall shape leans towards a slightly rounded elliptical form rather than a highly elongated shape.
