The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central region that gradually diffuses outward. There is little evidence of spiral arms or a well-defined disk. The color appears to be a relatively uniform yellowish hue, suggesting an older stellar population with lower rates of ongoing star formation, likely dominated by redder stars. The galaxy's overall round shape indicates a relaxed system that has undergone significant dynamical evolution. There is a hint of a minor disturbance in the morphology. The galaxy appears relatively isolated, without signs of major mergers or interactions with other galaxies in its immediate vicinity.
