The galaxy presents a somewhat elongated, intermediate morphology between a spheroid and a flattened disk structure. The central region appears relatively smooth and featureless with a high concentration of light, suggesting an older stellar population. Moving outwards, there is a subtle transition into bluer hues, particularly on one side, hinting at ongoing star formation activity within a disk component. There is some evidence of minor disturbances in the galaxy’s morphology; the asymmetry of the blue region could indicate gravitational interactions or past mergers.
