The galaxy presents an elongated morphology, likely a disk galaxy seen nearly edge-on. A prominent central bulge is apparent, exhibiting a bright, yellowish hue, suggestive of an older stellar population. The disk component appears relatively smooth, with minimal visible substructure like spiral arms. The light distribution within the disk is somewhat diffuse, fading gradually away from the bulge. The color of the disk appears to be slightly bluer than the bulge. The galaxy shows no obvious signs of recent major merger activity, although there are subtle signs of a minor disturbance in the galactic disk. Overall, this galaxy appears to be a relatively quiescent disk galaxy with evidence of past or ongoing, albeit low levels, star formation activity.
