This galaxy exhibits a disk-like morphology, presented edge-on from our vantage point. A prominent bulge dominates the central region, displaying a smooth, rounded structure and a yellowish hue, suggesting a population of older stars. The disk appears relatively thin and elongated, with dust lanes likely obscuring some of the starlight within it. The overall color gradient transitions from the warmer tones of the bulge to cooler, bluer hues towards the outer edges of the disk, possibly indicating ongoing star formation in these regions. There is no readily apparent presence of spiral arms or a bar structure. Minor disturbances might be present within the disk, but no major mergers are apparent.
