The galaxy presents as a centrally concentrated object, with a smooth, largely featureless appearance. The light profile suggests a dominant spheroid component, exhibiting a radial gradient in intensity that peaks sharply towards the galactic center. There is an elliptical morphology, verging on a spherical shape. Colors are consistent with an older stellar population, appearing reddish-yellow in the central region. A faint, bluish halo extends outward, although the contrast is minimal, suggesting low levels of on-going star formation. No spiral arm structure, bar, or distinct dust lanes are readily apparent. There is no indication of recent or ongoing major merger activity; however, there is a slight asymmetry in the outer halo that could point to a minor disturbance. The galaxy appears relatively isolated, without evidence of close companion galaxies or tidal interactions.
