The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. Its morphology is generally round, with no discernible spiral arms or distinct features. The galaxy's color index indicates a population of older stars, giving it a slightly yellowish hue, but with hints of bluer wavelengths in its outer edges. No signs of active galactic nuclei or significant dust lanes are visible, suggesting that it has a relatively low star formation rate. The light distribution suggests that the galaxy has reached a dynamically relaxed state. No nearby companion galaxies or signs of tidal disruption are visible, suggesting that it is not currently undergoing a major merger. The galaxy may be a candidate for a lenticular galaxy, but its smoothness points to an elliptical galaxy.
