The galaxy presents as a relatively smooth, elliptical-like object. It has a concentrated central bulge, exhibiting a yellow hue. The light seems to fade out gradually from the center, with no distinct spiral arm structures visible. The overall morphology suggests a lack of significant recent merger events. The roundness indicates that the galaxy is not highly elongated or disc-like when viewed from our perspective. There are no apparent tidal tails or other signs of ongoing or recent major interaction with another galaxy. The galaxy is likely a massive galaxy that does not have a very high star formation rate.
