The galaxy exhibits a generally elliptical morphology, with an estimated radius of approximately 2.7 arcseconds. A bright, concentrated central bulge is evident, suggesting a possible supermassive black hole at the galaxy's core and a significant old stellar population. The disk appears relatively smooth, lacking prominent spiral arm structures. Some degree of disturbance, likely in the form of minor gravitational interactions, is suggested. The galaxy displays colors that indicate active star formation regions, and possible recent merger activity. The overall structure implies a potential transition stage between a disk galaxy and a more elliptical form, although no strong evidence for a major merger is observed.
