The galaxy presents as an elongated structure, strongly suggestive of an elliptical morphology, although a highly inclined disk galaxy cannot be ruled out. The central region exhibits a high surface brightness, appearing relatively smooth with a yellowish-white hue, indicating an older stellar population. Moving outwards from the core, the brightness decreases and the color shifts towards bluer tones, implying the presence of younger, hotter stars and potentially some ongoing star formation in the outer regions. The outer regions appear somewhat disturbed or irregular, exhibiting faint extensions, which may be evidence of tidal interactions or past mergers. The overall shape is significantly flattened, with a bar-like structure running through its central bulge. The presence of dust lanes is not immediately obvious from the image, but could be present in faint concentrations within the disk.
