This galaxy exhibits a somewhat disturbed morphology, possibly indicative of a minor merger event. The galaxy displays a diffuse, disk-like structure, though the disk is not well-defined. There appears to be a central bulge region. Patches of blue color are visible, potentially signifying regions of ongoing star formation, distributed throughout its structure, although the rate of star formation is subdued. Evidence of tidal tails or other significant distortions are subtle, but some asymmetries are noted, hinting at gravitational interactions. Overall, the galaxy's light is predominantly distributed in a relatively compact area.
