The galaxy presents as a concentrated, smooth object. Its overall shape is elliptical, exhibiting a high degree of central concentration. The light profile appears relatively featureless, lacking any distinct spiral arm structures or prominent dust lanes. The color gradient suggests a population of older stars dominating the galaxy's composition, with a hint of bluer light in the central region potentially indicating a small amount of on-going star formation. There are no signs of tidal disturbances or significant interactions with neighboring galaxies. The galaxy's morphology appears largely undisturbed.
