The galaxy presents as a relatively smooth, centrally concentrated system. It displays a subtle radial color gradient, transitioning from a somewhat bluer hue in the outer regions to a slightly redder core. The overall morphology appears elliptical or lenticular, lacking prominent spiral arm structures. The light distribution is fairly even with no noticeable distinct features. There are hints of minor disturbances in the light distribution, potentially suggesting past or ongoing interactions, but no definitive signs of a major merger or tidal tails are apparent. The galaxy appears moderately distant, exhibiting a small angular size, consistent with a redshift. The concentration of light is generally high, with a clear distinction between the central bulge and the surrounding halo. The color profile indicates that the stellar populations are relatively old, though there might still be ongoing star formation, especially towards the edges of the galaxy.
