The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated with a generally round shape. There is a noticeable lack of distinct spiral arms or prominent star-forming regions. The light distribution suggests a relatively old stellar population, indicated by a yellowish-red hue dominant in the central region. The galaxy's outer regions exhibit a gradual decrease in surface brightness. There is no visual evidence of any major ongoing merger activity or significant tidal disturbances in the immediate vicinity.
