The galaxy presents as a relatively smooth, centrally concentrated object. There is a somewhat defined central bulge region exhibiting a yellowish hue, suggesting an older stellar population. This bulge gradually fades into a surrounding, less concentrated disk. The disk component is bluer, indicative of ongoing or recent star formation activity. While generally smooth, subtle irregularities or faint patches within the disk hint at potential spiral arm structures, though they are not clearly defined. The overall shape appears slightly elliptical. There is no strong evidence of a major ongoing merger, but there is the suggestion of some mild internal disturbance, although this could be explained by internal galactic processes.
