The galaxy presents as a fairly smooth, rounded structure. There is a subtle color gradient visible across the galaxy's body, transitioning from a somewhat yellowish-green hue in the central region to a slightly redder tone in the outer areas. This may indicate differences in stellar populations, with potentially younger, hotter stars concentrated towards the core. The galaxy does not show any obvious spiral arm structures, bar features, or signs of major tidal disturbances. There appears to be a concentration of light within the core region. There is an indication of ongoing though subtle star formation activity. The general morphology suggests that this is a galaxy undergoing some degree of passive evolution.
