The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, featureless morphology. Its light profile suggests a concentrated central bulge that fades gradually into the outer regions of the galaxy. It appears remarkably round in shape. There is no obvious spiral arm structure or significant dust lane obscuration visible. The galaxy is colored yellowish-orange. This suggests a likely older stellar population, with a diminished amount of recent star formation activity. There are no signs of tidal disturbances or merging activity. Overall, it seems to be a relatively isolated, quiescent galaxy.
