The galaxy presents a generally smooth and centrally concentrated morphology. The light profile appears to be dominated by a bulge component, exhibiting a relatively high degree of central concentration. The object appears largely featureless with no apparent spiral arm structures or strong dust lanes visible. The galaxy exhibits a roughly elliptical shape, with the major axis only slightly larger than the minor axis. Color gradients appear minimal, suggesting a relatively uniform stellar population throughout the galaxy, with a slightly redder core. Star formation appears minimal. No signs of tidal disturbances or ongoing mergers are evident.
