The galaxy presents a generally smooth, elliptical morphology. There is no discernible spiral structure or bar. The galaxy is fairly compact, with a concentrated central region and a gradual fade towards the outer edges. Its color appears yellowish-white, suggesting a population of older stars with lower rates of ongoing star formation. There is no strong evidence of tidal tails or morphological disturbances suggesting recent major merger activity, though a slight asymmetry cannot be ruled out. The galaxy is relatively isolated within this field of view.
