This galaxy exhibits a generally smooth morphology, appearing elongated with a high degree of ellipticity. The color distribution indicates a concentration of older stellar populations towards the galactic center, evidenced by the yellow-orange hue, suggesting minimal ongoing star formation in the core region. There appears to be a faint, bluer component enveloping the central bulge, possibly indicating some residual star formation in a flattened, disk-like structure, although it is subtle. The galaxy's overall structure doesn't show any prominent signs of major disturbances or ongoing merger activity, although there may be some very minor asymmetry that could be indicative of a past minor interaction. The galaxy appears relatively isolated. The estimated size is small.
