The galaxy presents a largely smooth morphology, appearing relatively featureless in this observation. Its light distribution suggests a centrally concentrated structure, likely exhibiting a spheroidal or elliptical shape. The color profile indicates a mix of stellar populations, with a slightly bluer hue surrounding the central region, possibly indicating ongoing, though limited, star formation activity. The outer regions display a redder tone, suggestive of older stellar populations. No prominent spiral arms or distinct disk-like structures are discernible. There is no evidence of significant tidal disturbances or ongoing mergers.
