The galaxy presents a generally elliptical morphology, exhibiting a smooth and relatively featureless structure. The central bulge is prominent and displays a high surface brightness, suggesting a high concentration of stars. Moving outwards from the core, the light intensity gradually decreases, with no clear evidence of distinct spiral arms or prominent dust lanes. There appears to be a slight elongation of the galaxy along a particular axis, hinting at a possible degree of flattening. The overall color profile suggests a population of older stars.
