This galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy viewed nearly edge-on. The primary body of the galaxy exhibits a gradient in color and brightness, indicating varying stellar populations and dust content. A prominent bulge is observable at one end of the elongated structure, appearing as a concentrated, yellowish region. The bulge may indicate an older stellar population, while the elongated main body shows a distribution of younger, bluer stars. A faint, diffuse halo may be present, surrounding the primary galactic structure, but it's indistinct due to the image resolution and contrast. There is a slight indication of tidal features or disturbances extending from the disk, hinting at past or ongoing gravitational interactions.
