The galaxy appears as a centrally concentrated system, elongated in shape, with a smooth, diffuse light profile. The central region is a bright, concentrated yellowish-white, suggesting an older stellar population. Moving outward from the center, the color transitions to a bluer hue. The galaxy lacks any discernible spiral arm structures or dust lanes, and appears to be a relatively undisturbed system. It shows features of a smooth galaxy, leaning to the shape of a rounded disk. There are no signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity, though some minor disturbances could be occurring. The observed colors imply a relatively low ongoing star formation rate within the galaxy.
