The galaxy presents a complex morphology, exhibiting a moderate degree of central concentration with an overall elliptical shape. The light distribution suggests a relatively smooth profile, though a faint, disturbed feature, possibly a tidal tail or merging companion, is suspected along one edge. The galaxy’s color index indicates a population of older stars, as evidenced by its reddish hue. The overall structure suggests that this galaxy is potentially undergoing or has undergone a merging event, further characterized by the tidal tail. The central region is bright, though the overall star formation rate is relatively low.
