The galaxy presents an elliptical morphology, though it appears somewhat flattened. A central bulge is visible, exhibiting a concentrated, bright, yellowish-white hue suggesting an older stellar population. Surrounding the bulge is a less concentrated disk. This disk presents a bluer color, hinting at the presence of younger, hotter stars and potential ongoing star formation. The overall structure appears relatively smooth, with only subtle hints of irregularities or disturbances, implying no major ongoing merger activity, but potentially some minor interactions. The galaxy appears to be moderately large in size.
