The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing mostly rounded with minimal elongation. A bright central bulge dominates the light profile, transitioning gradually into a more diffuse halo. There is a subtle color gradient, with the central region exhibiting warmer tones and the outer regions appearing cooler. No significant spiral arm structures or prominent dust lanes are discernible in the image. There is no apparent evidence of any major ongoing merger activity or strong tidal disturbances. Based on these morphological characteristics, this galaxy is likely an elliptical galaxy with relatively low star formation rate, possessing a considerable stellar mass.
