The galaxy presents a moderately bright, somewhat amorphous morphology. The central region exhibits a higher surface brightness, appearing as a diffuse, concentrated core. There is a subtle elongation visible, suggesting a deviation from a perfectly spherical shape, potentially leaning towards an elliptical form. The color profile indicates a dominance of intermediate-age to older stellar populations, with a hint of bluer regions that may indicate ongoing, but not vigorous, star formation activity. No distinct spiral arm structures or bars are discernible. There are some faint hints of a disturbed structure, perhaps indicating a prior interaction with another galaxy. Overall, the galaxy appears to be an intermediate-mass system undergoing a moderate level of star formation.
