The galaxy presents a generally smooth, elliptical morphology with minimal discernible structure. The central region is characterized by a concentrated, bright core exhibiting a yellow-orange hue, suggestive of an older stellar population. The light smoothly transitions into an extended, less luminous halo. The halo exhibits a subtle shift toward a redder color, with hints of blue suggesting the presence of a younger stellar population, albeit at a low star formation rate. No distinct spiral arms or bar structures are apparent. There is no visual indication of any major ongoing merger activity or significant tidal disturbances in its immediate vicinity. The galaxy appears primarily isolated.
