The galaxy presents as a flattened, disk-shaped structure. Its orientation appears nearly edge-on. The central region exhibits a higher surface brightness, appearing as a concentrated bulge. The color gradient suggests a relatively smooth stellar population distribution. There's a subtle color difference between the bulge and the outer disk, with the bulge showing a slightly yellower or whiter hue, indicative of older stars. Faint traces of blue light are visible in the disk region, possibly suggestive of ongoing star formation. There seems to be faint dust lanes within the galaxy's disk. There is no presence of strong spiral arms.
