The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, with a diffuse halo extending outwards. The light distribution is fairly uniform, with a noticeable color gradient, transitioning from slightly redder hues in the center to bluer tones in the outer regions. This may indicate ongoing star formation in the outer disk or halo. There is no clear evidence of spiral arms or a prominent disk structure based on visual inspection. The galaxy appears largely undisturbed, with no obvious signs of tidal interactions or recent mergers.
