The galaxy presents a relatively smooth morphology, appearing largely featureless at this resolution. Its shape is predominantly round. There is no obvious indication of major mergers or significant tidal disturbances. A slight colour gradient is observed, with a bluer hue towards the central region and a gradual shift toward redder tones in the outer parts, potentially indicating differences in stellar populations or dust content across the galaxy's structure. The galaxy appears to have relatively low ongoing star formation activity.
