The observed galaxy presents a disturbed morphology, suggestive of an ongoing or recent interaction. The primary structure exhibits an elongated, somewhat amorphous shape, with a noticeable tidal tail extending from one extremity, likely resulting from gravitational disruption. There is a prominent central bulge, appearing relatively bright and concentrated. The presence of multiple distinct clumps of light, primarily concentrated near the core, suggests localized regions of intense star formation activity, probably triggered by the interaction event. The overall color is on the redder end of the spectrum, implying an older stellar population. There seems to be a weak bar feature in the center. A slight disk structure, seemingly oriented edge-on, is also observable. However, the features may be a result of the galactic merger. It appears the galaxy may be a late-stage merger system.
