The galaxy appears as a centrally concentrated, smooth structure. Its shape is generally round, with hints of ellipticity. The light distribution suggests a dominant bulge component, typical of an early-type galaxy or possibly a spiral viewed face-on. The galaxy presents with a bluer color profile, suggestive of ongoing, or recent star formation. There is no clear evidence of spiral arms or a prominent disk, making classification difficult based on morphology alone. No significant tidal features or distortions are observed, which would suggest major recent merger events. Light seems uniformly distributed, with no apparent active galactic nucleus or strong emission regions. The galaxy's morphology suggests it may be transitioning between a more actively star-forming phase to one of quiescence.
