The galaxy presents as a relatively smooth, elliptical structure. Its core appears as a bright, concentrated region of high luminosity, suggesting a substantial stellar density. A gradual decrease in light intensity is observed moving outwards from the core, transitioning into a more diffuse halo. The galaxy's shape is generally rounded, showing only a slight elongation, not conforming to a highly flattened disk-like morphology or cigar shape. There is no evidence of prominent spiral arms or significant dust lanes. Based on these characteristics, the galaxy appears to be of an early-type, specifically an elliptical galaxy, with little to no active star formation. The overall impression is of a gravitationally settled system approaching a state of equilibrium. No major tidal disturbances or merging signatures are observed in this image. However, there is a slight indication of a minor disturbance or interaction in the outer regions.
