This galaxy presents as an edge-on spiral system. A prominent bulge is visible, with an apparent rounded morphology. The disk appears relatively smooth and lacks any immediately obvious signs of strong spiral arm structure. There's a noticeable concentration of light towards the central bulge, which gradually diminishes towards the outer edges of the disk. The colors of the galaxy suggest a relatively old stellar population, particularly within the bulge, which exhibits a yellower hue. Faint hints of bluer light can be observed within the outer regions of the disk, potentially indicating ongoing star formation, though the overall rate appears subdued. No significant signs of tidal disturbances, major mergers, or active galactic nuclei are apparent. The galaxy appears relatively isolated.
