The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light profile. Its overall shape is elongated, displaying a cigar-like morphology, though tending towards round. The galaxy's color gradient indicates an aging stellar population, with a centrally concentrated yellowish hue that fades to redder tones in the outer regions. There is little evidence of spiral arm structure or significant dust lanes. The smooth and relatively undisturbed appearance suggests it is unlikely to be undergoing a major merger currently. Faint, blueish features are observed, indicating some low-level star formation may be present.
