The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. There is a slight elongation along one axis, though it is generally quite round. The color gradient suggests active star formation, with a bluer hue more prominent in the central regions, indicating a higher concentration of younger, hotter stars there. The outer regions exhibit a subtle transition towards redder hues. There does not appear to be evidence of any major mergers or tidal disturbances, with only slight irregularities visible. Overall, this appears to be a galaxy with a dominant smooth structure.
