The galaxy presents as a somewhat smooth, centrally concentrated object, with a morphology that leans towards elliptical. It exhibits a relatively symmetric light distribution, but with a subtle, irregular feature on one side, possibly indicating a minor disturbance or interaction. The galaxy displays a blueish hue, suggesting the presence of a population of young, hot stars, although the overall star formation activity appears to be relatively low or quiescent. The effective radius of the galaxy is approximately 1.7 arcseconds.
