The galaxy presents a moderately elliptical morphology. There is evidence of a relatively large central bulge component, but it does not appear to completely dominate the galaxy's overall structure. No obvious spiral arm structures are observed. It is difficult to discern the detailed internal structure beyond the bulge. The galaxy's color profile suggests a mix of stellar populations, with some regions appearing bluer, indicative of younger stars or ongoing star formation, and other regions appearing redder, suggesting older stellar populations. The overall appearance is slightly disturbed, possibly influenced by a past or ongoing merger event. This is further suggested by the irregular shape and deviation from a smooth, symmetrical profile. The galaxy presents a high degree of central concentration.
