The galaxy appears as a single, concentrated luminous object, suggestive of a relatively smooth and featureless morphology. The color profile indicates a higher intensity in the blue wavelengths. This could imply the presence of a significant population of young, hot stars within the galaxy, indicating some level of ongoing star formation. The overall shape is predominantly circular. There is no obvious evidence of spiral arms, bars, or other distinct structural features. No obvious signs of tidal disturbances or ongoing mergers are visible upon visual inspection, but deeper analysis would be necessary to confirm this. Given its apparent magnitude, it is likely a relatively distant object.
