The galaxy presents an elliptical morphology, with a smooth and somewhat diffuse appearance. The light profile appears relatively uniform across the main body, lacking prominent spiral arm structures. There is a slight elongation, not distinctly cigar shaped, but not perfectly circular. The core regions exhibit a yellowish hue, possibly indicative of an older stellar population dominating those areas. A faint greenish tint surrounds the central regions, perhaps arising from a degree of ionized gas. There is evidence of a potential ongoing merger or interaction, suggested by a slightly disturbed morphology and light asymmetry. The star formation rate is low, suggesting that star formation has largely ceased within the galaxy. The galaxy exhibits no apparent dust lanes or significant features indicative of recent or active star formation. Overall, the galaxy appears to be a relatively massive system, undergoing or having undergone a merger or interaction.
