The galaxy presents a relatively smooth morphology, with a slightly elongated, elliptical shape. There is a bright central bulge that appears yellowish, suggesting an older stellar population concentrated in the core. Fainter, bluish extended regions are observed around the bulge, which could indicate the presence of younger stars and ongoing star formation, although they are not very prominent. Possible minor disturbances and asymmetry can be observed, suggesting there might be some merging activity or tidal interactions. The overall colour suggests a mix of stellar populations, with a relatively high mass and low specific star formation rate.
