The galaxy exhibits a roughly elliptical morphology, though exhibiting clear signs of tidal disturbance and merging activity. The central region presents a bright, concentrated core indicative of a possible nucleus. Faint and irregular extensions are visible, suggesting ongoing gravitational interactions and possibly the presence of tidal tails or debris. The color profile indicates a slightly redder hue in the central regions, possibly due to older stellar populations or dust obscuration, while bluer tints are observed in the fainter outer regions, suggesting more recent star formation. The galaxy displays a somewhat complex and disturbed structure, with multiple luminous knots and asymmetries apparent. This suggests that the galaxy is actively undergoing, or has recently undergone, a significant merger event. Overall, this galaxy exhibits a dynamic and evolving system, likely shaped by gravitational interactions with one or more companion galaxies.
