The galaxy presents an overall somewhat smooth morphology, yet exhibits features indicative of a disk structure. There is a central bulge with a bright core, surrounded by a flattened disk. The disk appears to be inclined relative to our line of sight. There are signs of some minor disturbances in the disk structure, although it does not show any obvious signs of major mergers or significant tidal features. The galaxy appears to be a relatively massive system, showing notable star formation activity.
