The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. The dominant color is a yellow-red hue, indicative of an older stellar population with diminished star formation. There is a slight hint of bluer light in the outskirts of the galaxy, potentially suggesting a small amount of ongoing or recent star formation activity in these regions. There is no evidence of spiral arms, a prominent disk structure, or any major tidal disturbances in the image, suggesting that it has not undergone any recent major mergers. The galaxy appears relatively isolated, showing no obvious signs of interactions with neighboring galaxies. The object exhibits high degree of roundness.
