The galaxy presents as a somewhat amorphous structure with a discernible central bulge exhibiting a yellowish hue, suggesting a population of older stars. Surrounding this central region, there's a fainter, bluish-tinged halo or disk, potentially indicating regions of ongoing or recent star formation. The overall morphology appears to be disturbed, with hints of asymmetries or irregular features extending outward from the main body. There may be evidence of tidal interactions or minor mergers in its recent past. Although the image resolution is limited, there are hints of faint, diffuse extensions, which could be indicative of tidal tails or disrupted galactic material.
