The galaxy exhibits a flattened, elliptical morphology, with a clearly defined central bulge that appears bright and concentrated. The overall color suggests the presence of both older stellar populations, evident in the yellowish hue of the central bulge, and younger stars or ionized gas in the outer regions, indicated by a subtle bluish tint. There is limited evidence of significant spiral arm structure or prominent star-forming regions, implying a relatively quiescent star formation rate. The galaxy's shape suggests it is likely an inclined disk galaxy viewed at an angle or an elliptical galaxy with a somewhat flattened shape. There are some possible signs of minor disturbances present but they are very faint. The galaxy appears relatively isolated, exhibiting no immediate signs of a major interaction or merger with another system.
