The galaxy presents an elliptical morphology, appearing elongated in shape. The central region exhibits a high degree of luminosity, characterized by a concentrated bright core. Proceeding outwards from the core, the galaxy's luminosity gradually diminishes, displaying a smooth transition into the outer regions. There is minimal evidence of defined spiral arm structures or significant dust lane obscuration. The color profile indicates a dominance of older stellar populations, based on the reddish hue observed in the galaxy's overall light. The outer regions exhibit a slightly bluer tint relative to the core, which might signify the existence of modest star formation activity within these areas. There appears to be no signs of major ongoing merging events or tidal disturbances.
