The galaxy exhibits a generally smooth morphology with a slight elongation. The color gradient suggests a centrally concentrated, older stellar population, likely dominating the core region. Fainter, bluer components are visible toward the outer regions, potentially indicating more recent star formation activity, but these features are not strongly defined, hinting at low levels of ongoing star formation. The overall shape appears mostly round, leaning towards elliptical, and does not display obvious signs of a prominent spiral structure or major mergers. There are some subtle irregular features which may be caused by tidal effects. The galaxy seems to be a fairly quiescent system with a dominant bulge and a relatively faint disk.
