The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outwards from the center, a subtle color gradient is observable, transitioning towards a slightly bluer, greener tinge in the outer regions. This might indicate the presence of younger stars. No distinct spiral arms or bar structures are apparent within the galaxy's disk. There are no obvious signs of tidal disturbances or interactions with other galaxies, although very faint extensions could be subtle signatures of possible past interactions. Overall, the galaxy appears largely undisturbed and relatively quiescent.
