The galaxy presents as a concentrated, ellipsoidal structure with a relatively smooth overall appearance. A central, luminous core dominates the galaxy's morphology, exhibiting a yellowish-white hue suggestive of an older stellar population. Extending outward from the core, a fainter, greenish-blue halo is observed, potentially indicating regions of more recent star formation. The galaxy is primarily smooth, but subtle distortions or faint features suggest there might be minor disturbances within the galactic structure, possibly due to a past interaction or ongoing internal dynamics. The overall shape is moderately round, with only a slight elongation, though it may appear more oblong at higher resolutions. Overall, the galaxy appears to be a fairly massive system, likely dominated by evolved stars, but still retaining some ongoing star formation activity, as seen in the outer regions.
