The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, exhibiting a bright, relatively uniform core. Moving outwards from the core, the light intensity gradually decreases without any distinct breaks or spiral arm structures visible. There is a slight elongation in the shape, deviating somewhat from a perfectly circular appearance. The galaxy appears to be a mature system, with minimal evidence of active star formation, indicated by the lack of strong blue emission. The overall color is yellowish, suggesting an older stellar population. No signs of tidal disturbances or mergers are apparent.
