The galaxy presents as a moderately inclined, disk-shaped system. A central bulge component is evident, exhibiting a yellowish-white hue, suggesting an older stellar population. The outer disk appears elongated, with a bluer color indicative of ongoing star formation. The disk structure appears somewhat flocculent, with hints of spiral arm segments, although the arms are not well-defined. Dust lanes are subtly visible against the bulge and inner disk. Overall, the galaxy shows intermediate characteristics between a pure elliptical and a fully formed spiral, suggesting it's a lenticular or early-type spiral galaxy. The galaxy exhibits a relatively smooth profile, with no signs of major mergers or significant tidal disturbances.
