This galaxy exhibits a clear disk-like morphology, viewed nearly edge-on. A prominent central bulge is visible, displaying a yellowish-orange hue. The disk appears relatively smooth, suggesting a lack of strong spiral arm features or significant dust lanes. The color of the disk transitions to a bluer tint further from the core, indicative of younger stellar populations. Overall, the galaxy presents a morphology consistent with a relatively evolved spiral galaxy or possibly an S0-type lenticular galaxy, with moderate mass and an estimated low star formation rate. There is the suggestion of minor disturbances to the galaxy likely through minor mergers or gravitational interactions.
