The galaxy presents a generally smooth appearance with a slight elongation, suggesting a possible elliptical morphology or a disk galaxy viewed at an oblique angle. The color profile exhibits a central concentration of yellow-orange hues, which may indicate an older stellar population. A distinct, redder, and more compact structure is visible offset from the galaxy's main body, potentially indicating a satellite galaxy or a region of intense star formation obscured by dust. There is minimal evidence of distinct spiral arms or a prominent bulge. Overall, the galaxy appears relatively undisturbed, though the presence of the distinct red structure suggests potential gravitational interaction or recent accretion event.
