This galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical with a high degree of roundness, showing no discernable spiral arm structure or a prominent disk. The color profile is dominated by yellowish hues in the central region, suggestive of an older stellar population. There are no distinct signs of major disturbances or ongoing merging activity; however, minor irregularities cannot be ruled out at this resolution. Overall, the galaxy’s structure suggests it is a mature system with little current star formation activity.
