The galaxy presents an overall smooth appearance, with a central bulge that is brighter and more concentrated than the surrounding regions. The galaxy exhibits a slight elongation, appearing more cigar-shaped than perfectly round. There is some evidence of minor disturbances within the galaxy's structure, possibly indicating interactions or internal activity. Star formation appears to be relatively low within the galaxy, based on its color and morphology. The galaxy is likely a relatively massive system, and is a notable distance from our own galaxy.
