The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape is somewhat elliptical, appearing mostly round. The central region exhibits a bright, yellowish hue, suggesting a high concentration of older stellar populations. Moving outwards, the color gradually transitions to a slightly redder tint, possibly indicating a decreasing age of stars or a higher dust content in the outer regions. There is some suggestion of a disturbed morphology, possibly reflecting an ongoing or recent merger event. The galaxy's features are somewhat indistinct, consistent with a relatively large distance and smooth overall structure. There is no clear spiral arm structure.