The galaxy presents an overall ellipsoidal morphology. A central, diffuse bulge region is apparent, exhibiting a moderate concentration of light. The outer regions of the galaxy appear fainter and more diffuse, without distinct spiral arm structures. The color profile suggests a population dominated by older stars, showing a redder hue. There are no distinct signs of active star formation regions or dust lanes visible in the image, based on the lack of strong blue concentrations. The galaxy exhibits a moderate degree of smoothness in its light distribution, hinting at a likely classification as an early-type galaxy. A slight asymmetry in the outer regions might indicate minor tidal interactions or past mergers, although no prominent disturbances are readily apparent in the image.
