The galaxy presents an overall smooth morphology. A dominant central bulge region is observed, exhibiting a bright, concentrated light profile. There is evidence of a weak disk, subtly extended. The color gradient shows that the central region displays a greenish-white hue, indicative of younger stellar populations or potential active galactic nuclei activity. Outer regions of the disk structure show more red/yellow which likely means it consists of an older stellar population. There appears to be a possible minor disturbance or interaction occurring, as evidenced by a slightly irregular shape, along with faint tidal features or distortions. A small number of objects are embedded in the disk; these may be compact star forming regions.
