The galaxy presents as a slightly inclined disk galaxy. A prominent, relatively bright bulge dominates its central region, exhibiting a smooth, rounded morphology. The disk component appears elongated and relatively thin, suggesting an edge-on or near edge-on orientation. The disk shows subtle variations in surface brightness, potentially indicating the presence of spiral arm structures or dust lanes, though the image resolution makes definitive identification challenging. There appears to be a hint of a minor disturbance in the disk, perhaps due to a slight gravitational interaction. The color profile indicates a relatively old stellar population within the bulge, while the disk may possess a mix of older and younger stars. The galaxy appears to be moderately massive, actively forming stars, but with a relatively low specific star formation rate.