The galaxy presents as a relatively smooth, elliptical morphology. There is a centrally concentrated bulge with a yellowish hue, suggesting an older stellar population. No distinct spiral arms or disk-like features are discernible. The overall roundness of the object is quite high. There is little evidence of any ongoing mergers or major disturbances in the immediate vicinity of the galaxy, although the very faint outer regions might suggest minor tidal interactions. The galaxy exhibits a general color profile that indicates moderate levels of star formation, offset with a prominent population of older stars.
