The galaxy presents as a moderately bright object with an estimated effective radius of approximately 2 arcseconds. Morphologically, the galaxy appears to exhibit a generally smooth profile, though subtle features may be present upon closer inspection. The light distribution suggests a primarily spheroidal structure, and there appears to be a general roundness. There is tentative evidence of a minor disturbance or interaction that does not appear to be due to any merger activity. The galaxy's color indices indicate bluer light in the green and red bands, and the z band cannot be determined from the image. 
