The galaxy presents a smooth, elliptical morphology. It appears elongated, exhibiting a notable axis ratio. The central region displays a high surface brightness, suggesting a concentrated nucleus. The color profile indicates a redder hue, consistent with an older stellar population. No distinct spiral arms or features are discernible. The overall structure points towards a galaxy devoid of significant ongoing star formation. There is a slight suggestion of tidal disturbances, which would indicate a possible interaction with another galaxy.
