The galaxy presents a primarily smooth morphology, exhibiting a lack of distinct spiral arms or bar structures. The galaxy is elliptical in shape, appearing somewhat elongated. The light distribution reveals a centrally concentrated bulge that smoothly transitions into a less luminous halo. The core displays a yellowish hue, possibly indicating an older stellar population. Moving outward, the halo shows a slight shift towards reddish tones, which might suggest the presence of a population of evolved, cooler stars, or possibly some dust obscuration. There is no clear evidence of ongoing major mergers or significant tidal disturbances. Weak star formation is likely present.
