The galaxy presents a largely smooth morphology, with a concentrated central region. The overall shape appears elliptical or nearly circular, exhibiting a high degree of roundness. There is little to no evidence of spiral arm structures or prominent dust lanes. The color profile indicates a redder hue, suggesting an older stellar population. No signs of major mergers or significant tidal disturbances are observed, with the galaxy appearing relatively isolated and undisturbed. Based on the color and smooth structure, the galaxy is likely an elliptical galaxy that has largely ceased star formation.
