The galaxy presents as an edge-on spiral system. A prominent central bulge is visible, appearing somewhat rounded, with a concentrated luminosity suggesting a significant population of older stars. The disk component is elongated and thin, oriented near perfectly edge-on relative to the observer. The image reveals a smooth texture with a noticeable lack of distinct spiral arm structures. The morphology is typical of a disk galaxy with an established bulge. There is no apparent evidence of tidal interactions or merging events. Based on color indices, the galaxy exhibits characteristics indicative of relatively moderate ongoing star formation.