The galaxy presents a slightly elongated morphology, appearing nearly edge-on. Its color profile suggests a moderate mix of stellar populations. The central bulge exhibits a bright, concentrated core, potentially indicating an older, well-established stellar population. Fainter, bluer regions appear to extend along the galaxy's plane, possibly tracing areas of more recent star formation. Subtle dust lanes might be present, though the resolution is insufficient for definitive confirmation. There is a distinct red bulge on the left of the image, which may be part of the galaxy or potentially a separate object.
