The galaxy presents as a somewhat elliptical, though not highly elongated, structure. Its core exhibits a bright, concentrated luminosity, indicative of a dense stellar population, likely an older population. The color gradient transitions from a yellow-orange hue at the core to a slightly redder tint in the outer regions. This color suggests a declining rate of star formation from the core outward. The morphology suggests a smooth light distribution, lacking prominent spiral arms or significant dust lanes. There are hints of disturbances in the galaxy's structure. There may be signs of possible tidal interactions in the form of faint asymmetries. Overall, the galaxy appears to be a relatively massive and evolved system.