The galaxy presents as a slightly elongated, lens-shaped structure. The central region exhibits a concentrated, bright nucleus with a yellowish hue. A diffuse, less luminous disk surrounds the core, displaying a gradual fading of light intensity towards the outer edges. There appears to be a subtle color gradient across the galaxy, with the central region showing warmer tones compared to the cooler hues in the outer disk. The galaxy's overall morphology suggests an intermediate classification between elliptical and spiral, likely a lenticular galaxy viewed at an oblique angle. No distinct spiral arm structures are clearly discernible, but subtle irregularities in the disk's brightness distribution hint at possible underlying features. There is no indication of a major ongoing merger, although there may be minor disturbances, possibly due to a smaller companion galaxy, or tidal effects.