This galaxy presents a generally smooth morphology, with a predominantly elliptical or spheroidal shape. The light distribution appears concentrated towards the center, suggesting a well-defined nucleus or bulge. The color profile indicates a higher concentration of older stellar populations, exhibiting reddish hues at the core. Fainter, bluer extensions hint at the presence of some ongoing star formation or younger stars residing within the outskirts of the galaxy. Some slight asymmetry or irregularity can be observed, possibly indicating minor interactions or disturbances in its recent history. Overall, this appears to be a fairly evolved galaxy, potentially residing at an intermediate distance, with a moderate level of stellar mass.
