The galaxy presents as a centrally concentrated light source, suggesting a spheroid-dominated morphology. There is little indication of spiral arm structures. The galaxy exhibits a relatively smooth appearance, with no obvious signs of ongoing major mergers or significant tidal disturbances. The light distribution appears somewhat circular, although subtle deviations from perfect circularity may be present. Color gradients across the galaxy are subtle, trending toward slightly redder hues in the central regions. This might indicate an older stellar population towards the galactic center. The galaxy's overall luminosity suggests a system of substantial mass, indicative of a mature galaxy that has likely undergone significant stellar evolution.
