The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution appears to be fairly uniform, lacking significant spiral arm structures or distinct features. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population with lower levels of ongoing star formation. There is a slight asymmetry in the outer regions but it is not likely to be a merger. The galaxy is not perfectly round, and is instead somewhat elliptical in shape. There is no evidence of a strong dust lane or significant tidal disturbances.
