The galaxy presents as a fairly smooth, elliptical structure, although a slight asymmetry is observed. A bright, concentrated central bulge dominates the core region, exhibiting a yellowish hue that likely indicates an older stellar population. The outer regions of the galaxy display a more diffuse and bluish tint, potentially suggesting the presence of younger stars or ongoing, albeit subdued, star formation activity. There may be some indication of minor tidal disturbances in the galaxy's outskirts, though further investigation with deeper imaging would be necessary to confirm. The galaxy's overall morphology appears to be intermediate between a perfectly spherical and a highly elongated shape. It does not seem to be undergoing a major merger, but minor interactions cannot be ruled out.
