The galaxy exhibits a generally smooth morphology, although some features or disturbances appear to be present. The central region of the galaxy is the brightest, with a concentrated luminosity, suggesting a possible nucleus or core. The overall shape of the galaxy seems elliptical or lenticular rather than spiral. Color gradients are apparent within the galaxy, with the central region appearing bluer compared to the outer regions, which exhibit a reddish hue. The observed colors indicate a mix of stellar populations within the galaxy, with the central blue region potentially indicating ongoing or recent star formation, while the redder outer regions suggest older stellar populations. There are faint indications of minor disturbances or tidal features.
