The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a bright, concentrated core that appears nearly spherical. Moving outward from the core, the light gradually diffuses into a more elongated, albeit still smooth, halo. There are no apparent spiral arm structures or significant dust lanes visible. The color profile indicates a relatively blue hue, though this is primarily concentrated towards the central regions, suggesting the presence of a population of younger, hotter stars. There is little evidence of significant ongoing star formation in the outer regions. Slight irregularities in the outer halo suggest the possibility of minor tidal interactions or past merger events.
