The galaxy appears as a centrally concentrated object with a relatively smooth and rounded morphology. There is a slight ellipticity, but it is close to circular. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a color gradient, with a slightly bluer hue at the core transitioning to a redder shade in the outer regions. This may indicate an older stellar population dominating the outskirts, while the core is composed of younger stars. No significant signs of ongoing merging events or tidal disturbances can be identified. The object presents itself as a relatively isolated system with no clear interactions with nearby galaxies. The observed characteristics suggest a classification leaning towards an early-type galaxy, most likely an elliptical or a lenticular galaxy.
