The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. The core exhibits a high surface brightness, appearing nearly circular and bright yellowish-white. Moving outward, the color gradually shifts to a fainter, more diffuse yellowish-white, indicating a possible decline in the stellar population density and/or a change in the dominant stellar populations. No distinct spiral arm features or prominent dust lanes are visible. The outskirts fade smoothly into the background sky, suggesting a gradual decrease in stellar density. There is no evidence of a significant tidal disturbance or ongoing major merger activity. A slight asymmetry may be present, though this is subtle. Overall, the galaxy appears to be a relatively quiescent system.
