The galaxy appears as a flattened disk, presenting an oblate spheroidal shape on the sky. The central region exhibits a pronounced bulge with a yellowish hue, suggesting an older stellar population. Moving outwards from the center, a bluer color is observed in the disk, indicative of ongoing or recent star formation. The disk itself shows some subtle irregularities, possibly signifying minor disturbances or interactions. The overall luminosity profile suggests a relatively large and massive galaxy. There are no obvious signs of strong tidal features or major mergers, but minor interactions cannot be ruled out based on the disk's morphology.
