The galaxy presents an overall bluish hue, suggestive of a relatively young stellar population or ongoing star formation. The morphology appears predominantly smooth and centrally concentrated, indicative of a possible elliptical or lenticular galaxy. However, faint extensions or irregularities are apparent in the outer regions, hinting at possible tidal interactions or minor disturbances. There is a clear decrease in magnitude from the G band to the R band, which aligns with the color. The galaxy appears to be of moderate angular size. A lack of redshift data limits further interpretation of its intrinsic luminosity and distance. Further observations would be needed to classify this galaxy more specifically.
