The galaxy appears as a relatively smooth, concentrated object, exhibiting an elliptical morphology. The central region presents a high surface brightness, diminishing gradually towards the outer edges. There is a slight elongation, suggesting a deviation from perfect circularity, tending towards a somewhat football shaped, but more likely in between round and football shaped. The color profile is generally uniform throughout the galaxy, displaying a yellowish-red hue, implying an older stellar population dominated by evolved stars, with a slight green tinge around the perimeter. No distinct spiral arm structures or significant dust lanes are discernible. There's no strong evidence of a major ongoing merger event, however, there appears to be some minor disturbances present on the lower edge of the disk. The overall appearance suggests a mature galaxy with a modest rate of star formation.
