The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, exhibiting a centrally concentrated light profile with a gradual decrease in brightness towards the outer regions. The galaxy's shape is predominantly round, displaying only minor deviations from perfect circularity. There is no strong evidence of spiral arms or prominent dust lanes. The color is dominantly yellowish-orange, suggesting an older stellar population, potentially dominated by evolved stars. Based on its color and smooth appearance, ongoing star formation appears to be relatively quiescent. There is no strong visual indication of any major ongoing merger activity or significant tidal disturbances, though minor disturbances cannot be ruled out based on the available data.
