The galaxy appears to be an elliptical galaxy, characterized by a smooth and diffuse light distribution. The central region of the galaxy exhibits a higher concentration of light. The object demonstrates a slightly elongated shape. No distinct spiral arms or prominent dust lanes are visible. The color appears relatively uniform, with a slight tendency towards redder hues, suggesting an older stellar population and suppressed star formation. The overall appearance indicates a well-evolved system. There is no indication of any major ongoing merging activity. There is a small chance of minor disturbances in the galaxy.