The galaxy presents as an elongated, disk-like structure, likely an edge-on or highly inclined spiral galaxy. There is a noticeable bulge component, exhibiting a yellowish-white hue, suggesting a population of older stars. The disk component appears blueish. The galaxy seems relatively undisturbed, showing little evidence of major mergers or tidal distortions. Faint hints of spiral arm structure might be present, but they are not very distinct and are largely obscured by the inclination. The overall morphology suggests a galaxy with an estimated stellar mass in the range of 10^8 - 10^9 solar masses and an active, moderate rate of star formation.
