The galaxy exhibits an overall elliptical morphology, though it is not perfectly symmetrical. The central region appears as a bright, concentrated core, suggesting a possible bulge component. The color profile of the galaxy shows variation. The core exhibits a bluer hue transitioning to a somewhat redder, fainter halo or outer disk region. Indications of faint, disturbed features are present in the outer regions of the galaxy, possibly hinting at minor tidal interactions or past merger events. The overall structure is predominantly smooth, though subtle irregularities suggest some level of morphological disturbance.
