The galaxy presents as an elliptical-like structure, with a dominant central bulge. The light profile appears smooth and centrally concentrated, exhibiting a relatively high degree of symmetry. The overall color is moderately red, indicative of an older stellar population and a lower rate of on-going star formation. No prominent spiral arms, bars, or distinct disk features are readily apparent. There is a very slight indication of a tidal disturbance or minor merger event, but any such feature is subtle. The galaxy is neither perfectly spherical nor exceptionally elongated; its shape is closer to being elliptical rather than disk-like, without a cigar-like morphology. The central core exhibits a brighter concentration, potentially associated with an active galactic nucleus or a region of enhanced stellar density. 
