The galaxy presents as a somewhat rounded, single, centrally concentrated object. There is no obvious spiral structure or a defined disk. The light profile appears smooth, with a gradual decrease in intensity from the core outwards. The galaxy exhibits a yellowish-orange hue, which may indicate an older stellar population and a relative lack of ongoing star formation. There is no apparent ongoing major merger or significant tidal disturbance of the galaxy's morphology. The object is relatively compact in size.
