The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The galaxy appears as a diffuse, elliptical object, displaying a relatively round shape. The color profile suggests an older stellar population, with a yellowish core region that gradually transitions to a bluer hue in the outer regions. No distinct spiral arm structures or prominent dust lanes are readily observable. There is no apparent ongoing merger activity or strong tidal disturbances in its immediate vicinity. The overall texture hints at a lack of significant star formation.