The galaxy exhibits a roughly elliptical morphology, appearing somewhat diffuse and lacking a clearly defined spiral structure. Its overall color is bluish, suggesting the presence of a population of young, hot stars and ongoing star formation, although at a low rate. There appears to be some disruption or feature within the galaxy, possibly a tidal feature, but the resolution limits a more detailed analysis. The light is moderately concentrated towards the center, suggesting the potential of a small bulge or nucleus. The galaxy's surface brightness is relatively uniform across its extent, indicating a fairly consistent stellar population density.
