The galaxy presents a predominantly smooth, elliptical morphology with a relatively high degree of roundness, though deviating somewhat towards an intermediate shape. There's an absence of clearly defined spiral arms or a prominent disk structure. The galaxy displays a color gradient, transitioning from bluer hues in the central regions to redder tones towards the outer edges. This color gradient could suggest variations in stellar populations, with younger, bluer stars concentrated in the core and older, redder stars dominating the periphery. While appearing mostly undisturbed, there is a subtle hint of asymmetry or minor perturbation in its overall shape, possibly indicating a past minor interaction.
