This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, centrally concentrated light distribution. The morphology is elongated, with a clear major axis significantly longer than its minor axis. The core of the galaxy is bright and appears bluish, possibly indicating the presence of a population of young, hot stars, or active galactic nuclei. The outer regions of the galaxy exhibit a redder color, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are visible. There is no evidence of a major merger, though subtle asymmetries or faint tidal features cannot be ruled out without further investigation. The galaxy is isolated, with no obvious signs of interaction with nearby galaxies.
