The galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge that transitions gradually into a less defined halo. The overall shape approximates an elliptical form, although there are some deviations from perfect sphericity. The central region displays a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color gradually shifts towards a redder tint. No prominent spiral arms or significant dust lanes are discernible. There is faint evidence of some minor disturbances in the outer halo. Overall, the galaxy appears relatively quiescent, with a low rate of star formation.
