The galaxy appears to be a relatively smooth and rounded structure, presenting a somewhat elliptical morphology. The core region of the galaxy exhibits higher luminosity, indicative of a concentrated stellar population or active galactic nucleus. The overall color profile suggests a mature stellar population. The galaxy exhibits a subtle asymmetry in its outer regions, which could indicate the presence of minor tidal disturbances or past interactions. Further investigation is needed to confirm the origin of this morphological feature.
