The galaxy presents as a moderately elongated structure with a noticeable central bulge. The disk exhibits a mottled texture, suggesting a degree of inhomogeneity in its stellar population and/or dust distribution. The color gradient across the galaxy is subtle, with a slightly bluer hue apparent in the disk regions compared to the redder central bulge. This might indicate ongoing star formation in the disk. The overall structure lacks well-defined spiral arms; rather, the morphology appears somewhat irregular. The observed asymmetry could be indicative of past or ongoing interactions with another galaxy.