The galaxy presents an elongated morphology. A central, concentrated region is visible, displaying a yellowish-white hue, suggesting an older stellar population. Faint extensions emanate from this core, giving the galaxy a somewhat irregular shape. A segment of the galaxy is bluish in color. This galaxy appears to be experiencing some form of disturbance, possibly due to a past interaction or minor merger event, resulting in some disruption to its structure. The star formation rate is relatively low, indicating this is a somewhat quiescent galaxy.
