The galaxy appears to be a relatively smooth, elliptical galaxy. It presents with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The light gradually diffuses outward from the core, forming a halo with no readily apparent spiral arm structures or distinct features. There is a lack of significant blue light, indicating minimal current star formation activity within the galaxy, or a very low specific star formation rate. The galaxy displays a rounded morphology, with no obvious signs of tidal disturbances or ongoing major merger events. There is a possible minor disturbance in the outer halo.
