The galaxy presents as a relatively smooth, elliptical form, elongated along a major axis with an approximate aspect ratio of 3:1. The light distribution suggests a central concentration of luminosity, with a gradual decrease in surface brightness extending outwards. There is a noticeable color gradient, transitioning from a more yellowish-white core region to bluer fringes at the periphery. This color change suggests potential differences in stellar populations between the inner and outer regions, perhaps indicating ongoing or recent star formation in the outer parts of the galaxy. There is no evidence of spiral arms or a distinct disk component. Close inspection does not reveal any strong evidence of ongoing major merging events. The overall morphology suggests an evolved system, likely an elliptical galaxy undergoing some form of ongoing, mild star formation activity, potentially triggered by a minor interaction or internal processes.
