The galaxy presents as an elongated, disk-shaped structure seen nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, potentially indicative of an older stellar population. The disk itself appears relatively smooth with no apparent spiral arm structure. Fainter bluish light is observed in the outer edges of the disk, possibly signalling regions of recent, albeit minimal, star formation activity. There is no evidence of any major ongoing merging events or significant tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed, massive disk galaxy.
