The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be fairly compact with a high degree of central concentration of light. There is a noticeable redder hue overall, with a slightly brighter central region, suggesting an older stellar population. No distinct spiral arms or significant dust lanes are discernible, further indicating a lack of active star formation. There appears to be minimal disturbance in its overall structure, implying that it is not currently undergoing a major merger. The object exhibits a roughly circular morphology, although with some minor deviations from perfect sphericity.
