This galaxy appears to be a relatively smooth, elliptical galaxy. The central region exhibits a concentrated and brighter luminosity, suggesting a higher density of stars and potentially an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases. The galaxy's overall color appears to be somewhat redder/gold, indicative of an older stellar population with a lower rate of star formation. The galaxy presents with a somewhat elongated, cigar-like shape rather than perfectly circular symmetry. There is little to no visible evidence of ongoing mergers or major disturbances in its structure, although there are some slight asymmetries to the halo.
