The galaxy presents as a spiral, exhibiting a centrally concentrated bulge that graduates into a more diffuse disk. The bulge displays a yellowish hue, potentially indicative of an older stellar population. The disk component shows faint spiral arm structures with bluer tones, suggesting ongoing star formation regions. The galaxy appears relatively undisturbed, without prominent signs of major mergers or tidal disruptions, although minor distortions in the outer disk are not entirely ruled out. Overall, the galaxy seems to have a relatively smooth morphology, with the bulge dominating the light profile. The system has a moderate redshift, placing it at a significant cosmological distance.
