The galaxy presents a largely smooth morphology with a central, brighter core region that diffuses outward. It appears to be elliptical in shape, deviating slightly from perfect circularity. The color gradient suggests a dominant population of older stars in the core, exhibiting a yellowish to reddish hue. There is little indication of spiral arms or significant dust lanes. Faint bluish tinges appear at the outskirts of the galaxy, suggesting the possibility of some younger stellar populations in the outer regions, or perhaps a region of ongoing low-level star formation. There is no obvious evidence of any major mergers or significant tidal disturbances; the structure appears generally relaxed and undisturbed.
