The galaxy presents as a somewhat diffuse, elongated structure. It appears to possess a bright, concentrated central bulge, surrounded by a fainter, more extended halo. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions display a bluer tint, suggesting the presence of younger, hotter stars. The overall form is suggestive of a disk galaxy, though the disk structure is not sharply defined. There's a slight indication of asymmetry or a minor disturbance in the outer regions, which could point to past interactions or a minor merger event. The galaxy's light profile gradually fades into the background, indicating no sharp edges or truncations in the stellar distribution.
