The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. The central region exhibits a concentrated, bright yellowish-white core, indicative of a high stellar density and potentially an older stellar population. Surrounding the core, there's a more diffuse halo of similar color, fading gradually outwards. Faint hints of bluer regions are observed in the surrounding area, suggesting the presence of younger, hotter stars or star forming regions, albeit minimal. Overall, the galaxy appears well-defined with no apparent signs of significant tidal disturbances or ongoing major mergers. The galaxy's shape is generally rounded.
