The galaxy appears as a centrally concentrated, elliptical system. It presents a smooth, featureless morphology, lacking prominent spiral arms or a distinct bar structure. The light profile suggests a relatively uniform stellar population with minimal dust obscuration. The overall shape leans towards an elliptical rather than a spherical configuration. There's no apparent ongoing merger activity or signs of tidal disturbances. The color index suggests a relatively evolved stellar population. The estimated size of the galaxy is approximately 4 kpc, indicating a small to intermediate size. Overall, the galaxy appears to be a quiescent elliptical system, consistent with a relatively old stellar population and a lack of significant star formation.
