The galaxy presents a generally smooth morphology, with a notable absence of clearly defined spiral arms. The shape appears elongated, possibly cigar-shaped, indicating a potential classification as an elliptical or lenticular galaxy viewed at an angle. The central region exhibits a bright, concentrated bulge, which is likely composed of older stellar populations, based on its yellowish-orange color. The outer regions show a bluer hue suggesting the presence of younger, hotter stars, indicative of some ongoing, albeit possibly low-level, star formation within a disk-like component or extended envelope. There is a faint hint of subtle disturbance or asymmetry in the outer disk, suggesting possible past interactions or minor mergers. However, there is no dominating major merger occurring.
