The galaxy presents a generally smooth appearance, with a slight elongation suggesting an elliptical morphology or possibly a disk viewed at an angle. The central region exhibits a bright, concentrated core, indicative of a high stellar density. Moving outwards, the galaxy shows a gradual decrease in luminosity. There are hints of color gradients within the galaxy, with the central region appearing more yellow, perhaps indicating an older stellar population. A subtle color change towards the outer edges exhibits a faint blue hue, possibly suggesting the presence of younger, hotter stars. There are no readily apparent signs of spiral arm structure, major dust lanes, or significant tidal disturbances. Based on the overall morphology, the galaxy is likely to be an early-type spiral or elliptical galaxy undergoing low levels of star formation.
