This galaxy appears to be an elliptical galaxy, exhibiting a largely spheroidal morphology. The light distribution is smooth and concentrated towards the center, indicating an older stellar population. There is little evidence of spiral arms or distinct features typically associated with disk galaxies. The core of the galaxy exhibits a yellowish hue which fades towards the edges into a slightly greener tinge, likely reflecting the distribution of stars within the galaxy. The overall structure seems undisturbed, with no signs of major mergers or tidal distortions. Minor disturbances may be present. The galaxy exhibits a relatively high degree of roundness.
