The galaxy presents an elliptical morphology, displaying a largely smooth light distribution with a slight deviation from perfect circularity. A concentration of light is observed towards the central region, indicative of a galactic nucleus. The galaxy exhibits a color gradient, transitioning from a yellow-ish hue in the central regions to a bluer tint in the outskirts. There is evidence of a possible merger with a smaller object in the lower right quadrant. This secondary object exhibits a higher concentration of bluer light. Overall, the galaxy appears to be fairly compact.
