This galaxy exhibits a flattened, elliptical morphology, appearing as a disk oriented approximately edge-on relative to our line of sight. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a high stellar density and potentially an active galactic nucleus or intense star formation within the core. The disk component shows some evidence of spiral structure, though it is somewhat faint and difficult to discern definitively. The color profile indicates a redder hue, implying a population of older stars and/or significant dust obscuration. The edges of the disk appear relatively smooth. There are some small regions of possible star formation in the disk, though not as significant as the luminosity of the central bulge. The overall structure suggests a galaxy that may be in a relatively evolved state.
