The galaxy presents as a relatively smooth, elliptical or lenticular structure. The core region exhibits a high degree of luminosity, characterized by a yellowish-white hue, possibly indicating an older stellar population and minimal dust obscuration. The galaxy appears more elongated than circular, trending towards a cigar shape. Faint, diffuse extensions are subtly visible beyond the bright core, suggesting the presence of a broader stellar halo. There is no clear evidence of prominent spiral arms or active star formation regions in this image, it appears to be in a relaxed state, with no major disturbances or signs of an ongoing merger event. Faint blue tones extend out from the core region indicating some star formation may be present.
