The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. There's minimal visible disk structure or spiral arms. The color profile suggests an older stellar population, with a yellowish hue dominating. A faint, extended halo might be present, though difficult to ascertain with certainty due to the image quality. There are potentially signs of minor disturbances or interactions, evidenced by slight asymmetries or faint tidal features, but these are not prominent, and the galaxy presents as largely undisturbed. Based on the colors and morphology, star formation is either suppressed or occurring at a very low rate. The overall shape is fairly round, with only a minor elongation visible. There are no distinct signs of a major ongoing merger.
