The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light profile, with a bright, diffuse core that decreases in intensity outward. The galaxy appears somewhat rounded in shape. There are hints of minor disturbances in its outer regions, though no major mergers or tidal tails are clearly visible. Color gradients are subtle, with the core exhibiting a slightly redder hue than the outer regions. Overall, the galaxy seems to be a moderately massive system with relatively low star formation activity.
