The galaxy appears to be an edge-on spiral galaxy, exhibiting a prominent, flattened disk oriented nearly perpendicular to our line of sight. The central bulge is quite bright and displays a rounded morphology, suggesting it is likely composed of older stellar populations. The disk itself appears smooth and relatively featureless, lacking prominent dust lanes or distinct spiral arm structures that are usually seen in spiral galaxies. There is a gradual fading in luminosity from the central bulge towards the outer edges of the disk. The overall color profile suggests a redder central region with a higher concentration of older stars and a bluer disk, indicating the presence of younger, hotter stars within the disk component. There is no evidence of recent major merging events or strong tidal disturbances.
