The galaxy presents as a smooth, elongated structure, appearing cigar-shaped when viewed. It exhibits a central bulge that appears more concentrated and luminous. There is evidence of some internal structure, with hints of a disk component, although this is not the dominant feature. The galaxy displays a color gradient, with the central regions appearing more reddish/yellowish, potentially indicating older stellar populations or dust obscuration. The outer regions display a bluer hue, suggestive of younger, hotter stars. There does not appear to be evidence of significant tidal disturbances or interactions with other galaxies. The overall morphology suggests a galaxy undergoing or having recently undergone a period of moderate star formation, though is on the passive side.
