The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile suggests a lack of prominent spiral arms or distinct disk-like structure. There's a color gradient, transitioning from a yellowish-white core to a greenish-yellow outer region, indicating potential differences in stellar populations. The galaxy's overall shape appears moderately elliptical, deviating from a perfectly circular form. The outer edges of the galaxy are indistinct, blurring into the background sky. There is no noticeable evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity. The light distribution is consistent with an older, more evolved stellar population, but the greenish-yellow outer regions might suggest ongoing or recent star formation activity there.
