The galaxy appears as a largely homogenous, elliptical structure. The light profile is concentrated towards the center, with a smooth and gradual decrease in brightness outward. The color appears primarily yellow to orange, suggesting an older stellar population with a lack of significant recent star formation. There is no discernible spiral arm structure or distinct dust lanes visible within the galaxy's disk, further supporting its classification as an elliptical galaxy. There appears to be a slight elongation but the galaxy is mostly round. It shows no signs of merging or tidal disturbances.
