The galaxy presents a generally smooth appearance with a slight asymmetry. A central, bright, yellowish core region is visible. The extended halo surrounding the core displays a bluer hue, suggesting a stellar population younger than the core. A faint, reddish concentration is observed on the upper left side of the galaxy, potentially indicating a region of recent or ongoing star formation, although dust obscuration cannot be ruled out. The galaxy's overall morphology appears to be somewhat elliptical, with an approximate diameter of roughly 6 kpc. There is no obvious presence of a spiral arm structure or significant dust lanes. Weak disturbance is possible on the left side of the galaxy.
