The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution suggests a fairly elliptical shape, though it leans towards being somewhat in-between round and elongated. The core region exhibits a bright, yellowish hue, potentially indicating an older stellar population. Surrounding the core, a more diffuse, bluish-white halo extends outwards. This suggests a component of younger, bluer stars, possibly indicating ongoing or recent star formation, though at a modest rate. There is little visual evidence of significant spiral structure, major disturbances, or ongoing mergers. Subtle irregularities may be present in the outer halo, which could suggest minor interactions or tidal effects, but these are not prominent. Overall, this galaxy appears to be a relatively undisturbed system.
