The galaxy presents as a relatively smooth, elongated structure. Its color gradient transitions from a concentrated reddish-orange core to a fainter, more diffuse yellowish-white outer region. The elongated shape suggests a possible classification as an elliptical galaxy viewed at an oblique angle, or a disk galaxy seen edge-on. There appears to be minimal evidence of distinct spiral arm structure or significant dust lanes within the limits of the image resolution. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal disruptions.
