The galaxy presents as an edge-on disk galaxy. A prominent central bulge is observed, exhibiting a concentrated, yellowish-white hue, suggesting a population of older stars. Extending outwards from the bulge, the disk component appears relatively smooth, lacking distinct spiral arm structures. The light distribution shows a clear elongation, further supporting the edge-on perspective. The disk appears dusty, with some evidence of blue star formation along the edges. A slight warping of the disk is not readily apparent at this resolution, nor is there any evidence of tidal features or major disturbances suggestive of ongoing mergers. The galaxy appears isolated.
