The galaxy appears as a slightly elongated, luminous object with a concentrated central bulge. Its overall structure seems relatively smooth with some subtle variations in color, the core displaying a yellowish hue that fades into a bluish-white aura towards the outer edges. This color gradient likely suggests differing stellar populations across the galaxy's structure, with older, redder stars concentrated towards the center and younger, bluer stars more prevalent in the outer regions. No distinct spiral arm structures are immediately discernible, leading one to assume this galaxy is likely elliptical, or potentially a smooth spiral galaxy viewed at an angle. Slight distortion in the halo may indicate interactions. The galaxy exhibits a moderate degree of star formation, given the bluish hue, indicating ongoing stellar production.