The galaxy presents a primarily smooth morphology, with a notable central bulge. A faint, diffuse disk component may be present, though not sharply defined. The galaxy exhibits a generally rounded shape. There is no strong evidence of ongoing major mergers, although the possibility of minor disturbances cannot be ruled out due to the presence of some asymmetry in the outer regions of the galaxy. The galaxy displays a range of colors, from a somewhat bluer hue in the outer regions to a redder color toward the center. This may indicate varying stellar populations, with younger, bluer stars in the periphery and older, redder stars concentrated in the bulge. Overall, the galaxy appears relatively massive and quiescent, with potentially low star formation activity.
