The galaxy presents as a somewhat elongated, disk-like structure. The central region exhibits a high degree of light concentration, appearing bright and yellowish-white, suggesting an older stellar population. The disk component shows a fainter, bluish hue, possibly indicating regions of ongoing star formation, though not particularly prominent. Overall, the galaxy appears relatively smooth, with a lack of distinct spiral arms or other notable features. There may be a slight distortion visible in the shape, though it is not significant enough to suggest a major ongoing merger.
