The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The color profile indicates a redder, more evolved stellar population, particularly within the central region. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears nearly circular, suggesting a low inclination angle with respect to our line of sight. Evident asymmetries or tidal features are absent, indicating it is likely not undergoing major merger activity. However, the possibility of minor disturbances or past merger events cannot be entirely ruled out based solely on this image. The lack of strong blue color suggests low current star formation.
