The galaxy presents a predominantly smooth morphology, with a highly concentrated central region. Its overall shape appears close to circular. The radial color profile suggests a slight reddening towards the center of the galaxy, possibly indicating an older stellar population or higher dust concentration in the core. There is little to no apparent evidence of spiral arm structures or significant disk features. No ongoing major merging activity or strong tidal disturbances are discernible; however, there may be slight signs of minor disturbances.
