The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light distribution with no discernible spiral arm structure. The central region displays a high surface brightness, suggesting a dense stellar population or active galactic nucleus. The overall color appears relatively uniform, trending towards a slightly redder hue, indicative of an older stellar population with lower rates of star formation. There may be some dust but it seems to be rather featureless. The galaxy appears relatively isolated, without strong tidal features or obvious interactions with neighboring galaxies. The galaxy's light profile appears circular and symmetric, suggesting that there is no merger happening, but there may have been a minor merger sometime in the past.
