The galaxy presents as a relatively smooth, elliptical structure. Its morphology is dominated by a spheroidal component, exhibiting a centrally concentrated luminosity profile. The color gradient suggests a possible presence of older stellar populations, particularly towards the galactic core, displaying a yellowish hue. There is no clear evidence of spiral arms or a prominent disk structure. A slight asymmetry in the outer regions might indicate a minor interaction, though the overall appearance is generally undisturbed. Star formation appears relatively quiescent across the galaxy.