The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape approximates a circle, with a slight deviation towards an elliptical form. The color profile indicates a dominant blue hue in the central region, suggesting the presence of a population of young, hot stars or an active galactic nucleus. There's a subtle color gradient towards the outer edges, showing hints of redder tones. These outer regions are less defined, possibly indicating a lower stellar density or a population of older, cooler stars. No strong spiral arm structures are apparent, nor are any obvious signs of tidal disturbances or ongoing major mergers, though there is a slight asymmetry visible that may indicate a minor disturbance.
