The galaxy presents as an intermediate-sized spiral galaxy with a noticeable central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The disk component is visible, though it is not highly resolved. Faint spiral arm structures can be discerned, appearing somewhat disrupted. The galaxy's overall color gradient transitions from the warmer tones of the bulge to cooler, bluer tones in the outer disk, indicative of ongoing star formation in these regions. There is some indication of minor disturbances in the morphology, possibly due to a past interaction or merger. The galaxy appears moderately inclined relative to our line of sight, giving it an elliptical appearance.
