The galaxy presents a generally smooth morphology. It exhibits a concentrated, elliptical shape, appearing nearly circular. The light distribution appears to be relatively uniform across the galactic body, lacking prominent spiral arms or a distinct central bulge. There appears to be a slight asymmetry in the light distribution, hinting at a possible minor disturbance or interaction. The galaxy's color suggests an older stellar population with a relatively low rate of star formation. There is no obvious dust lane or regions of intense, recent star formation visible. No companion galaxies or tidal tails are readily apparent, suggesting that any merger or interaction event is either in its early stages or concluded in the past.
