The galaxy presents as a single, relatively smooth and luminous object. It has a centrally concentrated brightness profile with a slightly elongated shape. There is a notable lack of distinct spiral arms or prominent dust lanes; however, there is a very faint, subtle extension projecting from the main body of the galaxy, suggesting possible tidal interactions or a very minor disturbance. The galaxy's color appears to be skewed towards the red end of the spectrum, indicative of an older stellar population. This suggests a lower rate of on-going star formation. The relatively smooth appearance and redder color suggest a classification leaning toward an elliptical galaxy.
