The galaxy presents a predominantly smooth morphology, with a slight elongation visible in its overall shape. The central region exhibits a concentrated luminosity, appearing nearly spheroidal with a yellowish hue, suggesting an older stellar population. Moving outward from the center, the galaxy displays a gradual decrease in surface brightness. There are hints of subtle structural features, possibly indicative of a weak disk component or spiral arms, although they are not sharply defined. The overall color gradient shifts towards a bluer tint in the outer regions compared to the core, potentially signifying regions of more recent star formation activity. There are no obvious signs of major mergers or strong tidal disturbances affecting the main galactic body.
