The galaxy presents a generally smooth, elliptical morphology. A discernible central bulge is present, appearing more concentrated and yellowish in color, suggesting an older stellar population. The outer regions exhibit a subtle disk-like structure, indicated by the slight flattening. A faint greenish hue is observed in these outer regions, possibly indicating ongoing, albeit weak, star formation. There's no strong evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a galaxy in transition, potentially moving from a spiral to an elliptical morphology, with relatively little ongoing star formation.
