The galaxy presents an overall flattened, disk-like morphology with a visible central bulge. It appears to be oriented roughly edge-on from our vantage point, with a projected major axis that is noticeably longer than its minor axis. The light distribution indicates a concentration of older stellar populations in the bulge region, based on the colors in the image.

A faint, extended halo or disk component is visible surrounding the central region, suggesting the presence of more diffuse stellar populations. There is some faint structure that could suggest minor tidal disturbances, but more data would be needed to make a conclusion. There appears to be some variation in the color, indicating a mix of stellar ages and/or dust obscuration patterns in the structure. Based on this, a possible classification could be a spiral galaxy viewed edge-on.
