The galaxy presents a flattened, elongated morphology, appearing nearly edge-on relative to our line of sight. The central bulge is prominent, exhibiting a bright, concentrated luminosity, with colors suggesting an older stellar population. Extending outward from the bulge, the disk is clearly visible, though its structure is not as sharply defined. Colors within the disk indicate the presence of both older stars and pockets of recent or ongoing star formation. The outer regions of the disk appear somewhat diffuse and less luminous compared to the central regions. The galaxy does not show any obvious signs of tidal disturbances or interactions with other galaxies. There is some indication of dust lanes within the disk, obscuring the light from background stars and gas. Overall, the galaxy appears to be a relatively undisturbed disk galaxy seen at a high inclination.
