The galaxy appears to be a relatively compact system with a bright, concentrated central region suggestive of a significant bulge component. Its overall morphology presents a somewhat smooth appearance, although there is a subtle indication of a disk-like structure surrounding the core. The colors present are indicative of a moderately active stellar population, though no strong indications of intense star-forming regions or prominent spiral arms are immediately apparent. There is a faint disturbance on the outskirts of the galaxy, it is possible that this is due to minor interactions with another galaxy. 
