The galaxy appears to be elliptical in morphology, characterized by a generally smooth light distribution without prominent spiral arms or a well-defined disk. There is a slight elongation visible, deviating marginally from a perfectly circular shape, with a central bulge. There is an absence of significant dust lanes or prominent star-forming regions, as indicated by the smooth, homogeneous color profile. There might be some minor asymmetry. No signs of tidal tails or major disturbances are observed, which suggests that it has likely not undergone any significant merger events recently. The galaxy exhibits a bluish hue, hinting at the presence of some young, hot stars or perhaps relatively high metallicity.
