The galaxy appears to be elliptical in morphology. The light distribution seems largely smooth and centrally concentrated, lacking prominent spiral arms or a significant disk structure. The galaxy's overall shape leans towards being moderately elliptical rather than perfectly spherical or highly elongated. There is a hint of minor structural disturbance present, possibly indicating a past or ongoing interaction with a smaller companion galaxy, but it appears generally relaxed. The core shows a higher concentration of light than the surrounding regions. The galaxy exhibits color variation, transitioning from a bluer hue in the central region toward redder hues at the edges.
