The galaxy presents a primarily smooth morphology, with a centrally concentrated light profile. The shape is somewhere between round and elliptical. There is an absence of defined spiral arms or a distinct disk structure. A minor asymmetry can be observed, but no major disturbances are evident. The galaxy exhibits a yellowish color, concentrated in the core, which fades gradually to a bluish hue in the outer regions. This color gradient suggests a possible difference in stellar populations, with the core likely populated by older stars, while the outskirts may contain a younger population. Overall, the galaxy appears to be relatively isolated, showing no clear signs of ongoing major interactions or mergers.
