This galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a centrally concentrated light profile. The main body of the galaxy presents a somewhat spherical shape, with a gradual decrease in luminosity from the core outwards. There is a subtle color gradient visible, transitioning from a bluer central region to slightly redder outer regions. This may indicate ongoing, albeit low-level, star formation, possibly more concentrated in the core. There is no apparent spiral arm structure or significant dust lanes. Minor disturbances may be present within the galaxy, but if so, they are quite minimal. Overall, this galaxy appears to be a settled system without evidence of recent major mergers or strong tidal interactions.
