The galaxy appears to be a spiral galaxy viewed at an oblique angle. It exhibits a generally smooth, elliptical profile with a bright central bulge that is more luminous than the surrounding disk. The bulge displays a yellowish hue, likely indicating an older stellar population. A flattened disk surrounds the bulge, showing hints of spiral arm structure. The arms are not well-defined, instead appearing as subtle variations in color and brightness within the disk. The disk exhibits a bluish tinge, suggesting the presence of younger, hotter stars and ongoing star formation. No major disturbances or tidal features are apparent, indicating that the galaxy is likely not undergoing a major merger event, though there might be very minor disturbances. Overall, the galaxy appears to be relatively isolated and unperturbed.
