The galaxy appears as a centrally concentrated, elliptical or lenticular system. It is largely featureless, exhibiting a smooth light distribution with no apparent spiral arms or bar structures. The core region displays a bright, yellowish-white hue, suggesting an older stellar population. The color becomes slightly redder moving towards the galaxy's outer regions, which suggests the possible presence of dust obscuration or an increasing proportion of older, redder stars within the galaxy's halo. There is no indication of any ongoing major merger activity or strong tidal features. Minor disturbances or faint plumes cannot be ruled out entirely given the image quality, but no prominent signs are observed. The galaxy's overall structure suggests a relatively evolved system with little ongoing star formation.
