The galaxy presents a largely smooth, elliptical morphology with no distinct spiral arm structure immediately apparent. The core exhibits a slightly brighter concentration of light, fading into a more diffuse halo. The color profile is suggestive of an older stellar population, dominated by redder wavelengths, although some bluer light is present. The overall shape appears somewhat rounded, though it deviates from a perfect circle, with some elongation. There's no clear evidence of ongoing major mergers or significant tidal disturbances, though faint asymmetry hints at a minor interaction in the past.
