The galaxy exhibits an elliptical morphology, appearing moderately elongated. Its color profile suggests a dominant population of older stars, presenting a yellowish hue. There is no clear evidence of spiral arm structures or significant dust lanes. The central bulge is prominent and relatively bright, indicating a high concentration of stars. The outer regions display a gradual decrease in luminosity, suggesting a smooth stellar density distribution. There's no obvious sign of ongoing major merging events or strong tidal distortions, although subtle irregularities may indicate minor past interactions. Overall, it is consistent with a relatively evolved galaxy, likely undergoing a lower rate of star formation.
