The galaxy appears to be an elliptical galaxy, presenting as a smooth, concentrated spheroid of light. The light is strongly concentrated in the center of the galaxy, indicating the possible presence of a supermassive black hole or a dense stellar population. The light distribution is remarkably homogenous across the central region, fading gradually towards the edges without any distinct spiral arm structures. The color is generally yellowish, suggesting an older stellar population with a low rate of ongoing star formation. There are no noticeable dust lanes or other significant features to indicate active galactic processes. There are no signs of interactions with other galaxies or evidence of recent merger events, maintaining the morphology of a generally isolated galaxy.
