The galaxy presents a generally smooth morphology, suggesting an elliptical classification, with no obvious spiral arms or distinct features of a disk galaxy. The central region displays a concentrated, bright yellow or golden hue, likely indicative of an older stellar population. The isophotes are generally elliptical, with a moderate ellipticity. There is a subtle extension of light beyond the central bulge, indicating a halo of stars. Faint blue regions can be spotted sporadically in the surrounding light, possibly representing new star formation within the galaxy. The galaxy shows no signs of major mergers or tidal disturbances, suggesting it is relatively undisturbed.
