The galaxy appears as a centrally concentrated object with a largely smooth light distribution, suggesting an elliptical morphology. The galaxy exhibits a pronounced spherical shape, with minimal deviation from perfect roundness. There is no discernible disk component or spiral arm structure visible in the image. The color profile of the galaxy is biased towards the redder end of the spectrum, indicating an older stellar population and suppressed star formation activity. There is no apparent evidence of on-going or recent major merger events, or strong tidal features. There may be evidence of a minor disturbance to the shape of the galaxy.
