The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. There is a concentrated central bulge, exhibiting a higher luminosity than the surrounding regions. The overall color profile suggests an older stellar population, potentially with a low rate of ongoing star formation. The galaxy is relatively isolated, with no apparent signs of major interaction or merging events. Its shape is close to circular, showing minimal elongation. Small traces of disturbances or faint disk like features are likely burried in the data.
