The galaxy presents an overall smooth morphology, appearing largely featureless. It exhibits an elliptical shape, with a moderate degree of elongation. The central region shows a concentrated luminosity, possibly indicating a galactic bulge. A faint bluish hue is observed in the galaxy's outer regions, suggesting the presence of younger, hotter stars undergoing active star formation, although this activity is likely low. Redder tones permeate the central regions. There are no obvious signs of a major ongoing merger, though subtle asymmetries might indicate past interactions or minor disturbances within the galaxy.
