The galaxy presents with a generally smooth morphology, exhibiting a central bulge that appears nearly spherical in projection. The light distribution suggests a degree of homogeneity within the central region. Fainter extensions are observed, possibly indicative of a weak disk or tidal features. The color gradient shows a yellowish center, potentially suggesting an older stellar population, transitioning to slightly bluer tones in the outer regions, indicative of possible ongoing star formation. There's a hint of asymmetry or slight disturbance in the overall structure, possibly the result of a minor interaction or internal dynamics. The object does not appear to be undergoing a major merger, although there may be hints of minor disturbances present.
