The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. There's a slightly elongated shape, but no prominent spiral arms or disk structures are discernible. The galaxy's core appears bright and yellowish-white, suggesting an older stellar population. Fainter, bluer light can be seen in the surrounding halo, indicating some ongoing, albeit low, levels of star formation. Minor disturbances can be identified, which may hint at tidal interactions. It does not appear to be undergoing a major merger.