The galaxy presents a largely smooth, elliptical appearance with a slight central concentration of light. It exhibits an overall round shape, with minimal deviation from circular symmetry. There is no obvious dust lane or spiral arm structure visible. The color profile suggests a general blueness, possibly indicative of ongoing, though not pronounced, star formation activity within the galaxy. There may be a minor disturbance, indicating a past merger or tidal interaction with a satellite galaxy, although there are no obvious signs of major disruption. 
