The galaxy presents as a flattened, disk-shaped structure viewed nearly edge-on.  It exhibits a strong central bulge component, characterized by a high degree of radial concentration and a yellowish hue, suggesting an older stellar population. The disk component appears relatively smooth with little discernible structure in the available imagery, indicating a lack of prominent spiral arms or significant star-forming regions.  The overall color profile indicates a galaxy dominated by older stars, with minimal ongoing star formation. There is no apparent evidence of a major merger event, although there is very slight irregularity that might imply the presence of minor tidal disturbances. Given the edge-on perspective, a significant amount of dust may be obscuring details within the disk.
