The galaxy presents as a luminous, elliptical structure. The central region exhibits a high degree of smoothness, with a concentrated core indicative of an older stellar population, likely dominated by evolved stars exhibiting a yellowish hue. Faint extensions are visible surrounding the central region suggesting a low level of disk structure, but are overall smooth. There is no strong evidence of any ongoing major merger activity or tidal disturbances. The galaxy appears relatively isolated, showing no immediately interacting companion galaxies or significant asymmetric features.
