The galaxy presents as a relatively smooth, elliptical structure. Its core is a bright, concentrated region exhibiting a yellow-white hue, suggesting a population of older stars. Surrounding this core is a less defined, more diffuse region extending outwards, tinged with a blue-green color. This outer region implies the presence of some younger, star-forming areas, although at a seemingly low rate. The galaxy appears to have an intermediate ellipticity, leaning towards a rounded shape rather than a highly elongated or cigar-shaped one. There are no clear indications of significant tidal disturbances or ongoing mergers, although a slight asymmetry may suggest a minor interaction in its past. The overall morphology points to a galaxy that has largely settled into a quiescent state.
